The galaxy presents as a relatively compact object with an overall smooth appearance, though subtle features are discernible. The main body is noticeably round. There is a suggestion of disturbed morphology, with some light that is off center. There appear to be two dominant concentrations of light, with a possible third light concentration that is more dim. This could be a potential merger. Color analysis reveals a redder hue towards the center, indicative of an older stellar population or dust obscuration, while the outer regions exhibit bluer tones, suggesting ongoing or recent star formation.
