The galaxy presents as a system of two distinct components: a larger, diffuse structure and a smaller, more compact feature.

The larger component exhibits a relatively smooth, elliptical morphology. Its core displays a higher surface brightness with a yellow-orange hue, suggesting a population of older stars. The outer regions of this structure are less luminous and exhibit a greenish tint. This color variation suggests a possible difference in stellar population, with potentially younger, hotter stars contributing to the green light, or may be indicative of ionized gas.

The smaller component consists of at least two, possibly three, compact, redder knots. These knots are less extended than the main galaxy body, and their color suggests an older stellar population and potentially high dust content. These knots could be star clusters or tidally disrupted dwarf galaxies interacting with the main system.

Overall, the galaxy's morphology suggests a system undergoing or having undergone some form of interaction. While the main body appears relatively undisturbed, the presence of the knots may indicate a past or ongoing minor merger event. Further spectroscopic data would be necessary to confirm the nature of the knots and their relationship to the main galaxy.
