The object appears to be a galaxy with a generally round morphology. The light distribution of the central region seems relatively smooth and concentrated. There is a suggestion of faint, diffuse material extending outwards from the central body. The color profile suggests that it may contain regions of both older stellar populations in the outer extensions and potentially a bluer, more active region in the core where there may be areas of active star formation. Evident are some signs of disruption or interaction, perhaps in the form of tidal tails or asymmetries in the outer regions. There are some indications of other structures possibly associated with an ongoing or previous merger event. The overall color suggests a significant population of older stars, with a possible component of younger stars in the core contributing to the bluer hue.
