The galaxy presents a generally smooth and rounded morphology, suggestive of an elliptical or lenticular type. It exhibits a bright, concentrated core, with a diffuse halo extending outwards. There are no apparent spiral arm structures or significant dust lanes visible. A secondary, slightly less luminous component is observed in close proximity to the primary galaxy, potentially indicating an ongoing or recent merger event. The overall color is yellowish, which could suggest a relatively older stellar population, with a low rate of ongoing star formation, and an estimated physical size of roughly 4 kpc. The system shows signs of disturbance, possibly due to the interaction with the companion galaxy. This is reinforced by the high liklihood of ongoing mergers of some kind within the galaxy.
