The galaxy presents as a relatively smooth, elliptical-like structure. It is centrally concentrated with a bright core region that appears almost spheroidal. The luminosity decreases gradually outwards from the center. The galaxy exhibits a blueish-white hue in its central and inner regions, suggesting the presence of a population of younger, hotter stars. The outer regions show a slightly more yellowish tone which would suggest an older stellar population. There is a distinct, smaller yellow or orange object in close proximity to the primary galaxy. The two may be interacting with each other. There are some subtle signs of distortions in the galaxy's overall shape, which might indicate tidal interactions or recent merger activity.
