The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a cigar-shaped morphology with a noticeable central bulge. The color profile suggests a population of older stars, with a redder hue concentrated towards the central region, which could imply ongoing or recent star formation at a low rate. There are some minor disturbances or asymmetric features present, but the galaxy does not show strong evidence of major mergers or tidal interactions. It appears relatively isolated in its environment.