The galaxy presents as a system with a dominant, relatively smooth central component. The primary body exhibits a yellow-orange hue, suggesting an older stellar population with minimal ongoing star formation. The overall form is generally rounded, with a slight elongation or irregularity suggesting a possible deviation from a perfectly elliptical shape. 

A secondary, smaller component is visible, displaying a bluer color, indicating the presence of younger, hotter stars and potential star-forming regions. This feature is notably less concentrated than the main body, giving it a diffuse appearance.

There are indications of possible tidal features or minor disturbances in the galaxy's morphology. This could signify interactions with other galaxies or past merger events, resulting in a more complex structure than would be expected in an isolated elliptical system. Further investigation would be needed to confirm the precise nature and origin of these features.
