The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core exhibits a yellowish-white hue, indicative of an older stellar population. Moving outward from the core, the surrounding region displays a slightly bluer tint, suggesting the presence of younger stars or ongoing star formation, though the overall star formation rate is low. There is a very slight distortion in shape indicating a possible tidal interaction with a neighboring galaxy at some point in the past.
