This galaxy exhibits an elliptical morphology, with a noticeable central bulge that appears quite bright and diffuse. There is little evidence of spiral arm structure. The color profile indicates a concentration of older stellar populations, as the galaxy exhibits a reddish hue overall, particularly towards its core, although blue light is visible in the surrounding halo.

There are some signs of possible interaction or disturbance, specifically a slight asymmetry in its shape and some faint tidal features potentially extending outwards. This could be indicative of a past or ongoing minor merger event. Overall, the galaxy appears relatively smooth with some subtle features hinting at past interactions.
