The galaxy presents as an elliptical-like morphology, exhibiting a centrally concentrated bulge. The color profile suggests a dominant population of older stars, indicated by the yellowish-red hue. There's little evidence of substantial dust lanes or active star formation regions, although faint bluish tinges are present around the perimeter and seem to be coming from a slightly distorted disk. Overall, the galaxy appears relatively smooth and undisturbed. There may be a small companion galaxy within close proximity.
