The galaxy presents a predominantly elliptical morphology, appearing as a smooth, concentrated spheroid of light. Its core exhibits a bright, yellowish hue, suggesting a significant population of older stars. A subtle, extended halo surrounds the central region, fading gradually into the background. 

There is a hint of asymmetrical structure. On one side of the galaxy, a faint, somewhat elongated feature can be discerned. It exhibits a slightly bluer color than the core, possibly indicative of a region with ongoing star formation. This feature could be a tidal tail or a minor disturbance resulting from a past or ongoing interaction with another galaxy.

Overall, the galaxy appears relatively isolated in its environment, with no immediately obvious signs of a major merger event, although subtle disturbances suggest a more complex history. The galaxy exhibits a moderately high mass. The red-yellow color suggests a relatively low star formation rate.
