This galaxy exhibits a generally smooth, elliptical morphology. The central bulge region displays a bright, concentrated luminosity. Moving outwards, there is a noticeable fading of intensity in the outer regions of the galaxy. The color profile suggests an older stellar population, indicated by the redder hues dominant in the central bulge. Fainter, bluer regions are visible, potentially indicative of areas of more recent star formation. There are potentially some minor disturbances with a possible interaction with another galaxy. The overall shape is roughly rounded with slight elongation. There is an absence of a distinct disk structure. Overall, the galaxy appears to be a fairly massive, early-type galaxy undergoing a relatively quiescent phase of stellar evolution.
