The galaxy presents an elliptical morphology, elongated along its major axis. Its central region exhibits a high degree of smoothness with a yellowish-white hue, indicative of an older stellar population. The outer regions show a less uniform texture, possibly due to the presence of dust or regions of more active, ongoing star formation. Faint spiral arm-like structures, though not clearly defined, suggest that it may be a lenticular galaxy seen at an angle. There is also some evidence of minor disturbances in the galaxy’s structure, which could indicate a past interaction with a smaller galaxy or tidal effects. There is no significant evidence for it undergoing a merger currently.
