The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. The light distribution is primarily concentrated towards the center, with a noticeable falloff in intensity towards the edges. There appear to be some subtle, extended features or distortions present that indicate the possibility of a galaxy interaction or ongoing merger event. There are three distinct high brightness points, implying either mergers or areas of intense star formation. The color profile is primarily redder, suggesting a population dominated by older stars and a relatively low current star formation rate. The galaxy has a mass on the high end.
