The galaxy exhibits a smooth morphology, likely elliptical, with a relatively high central surface brightness. It appears to be moderately massive. The light distribution suggests it is neither perfectly spherical nor significantly elongated; more of an intermediate shape. There is no obvious evidence of a major merger event, although there might be some minor disturbances in its structure. It appears to be actively forming stars, with the presence of some blue light indicating recent or ongoing star formation, but it could be dominated by older stellar populations given the overall color and smoothness. The galaxy is a considerable distance away from us.
