The galaxy appears to be a relatively small, smooth galaxy with a slightly elongated shape. It exhibits a centrally concentrated luminosity profile, appearing brightest near the core. There is little visible structure or distinct features, such as spiral arms or a prominent dust lane, indicating it may be a spheroidal galaxy. The color suggests that it is composed of older stars and is not undergoing significant active star formation, exhibiting a primarily redder hue with some regions that are blue. There is no obvious evidence of any major mergers or tidal disturbances. The object is most likely elliptical.