The galaxy presents as a system with a primary, relatively smooth component and a secondary, smaller feature likely interacting with it. The main component exhibits a diffuse, elliptical morphology. The light is concentrated towards the center, with an apparent color gradient suggestive of older stellar populations dominating the core. The outer regions show a bluer hue hinting at possible ongoing, albeit subdued, star formation activity. 

The secondary feature displays a more irregular shape. Its color appears similar to, if slightly bluer than, the outer regions of the primary galaxy. This feature is situated close enough to suggest it may be undergoing tidal disruption, leading to the disturbed morphology and potentially fueling the subdued star formation activity observed in the primary galaxy.
