The galaxy presents as a relatively compact, elliptical-like structure. It exhibits a smooth, concentrated light profile, with the majority of the light emanating from the central region. There is no readily apparent disk component or spiral arm structure. The color appears somewhat blue-white, possibly indicating a younger stellar population compared to purely elliptical galaxies, but this could also be due to redshift effects. No tidal features or strong indications of recent merger activity are immediately visible, though minor disturbances cannot be ruled out at this resolution. The galaxy's overall morphology suggests a system undergoing, or having recently completed, a transition towards a more quiescent, spheroidal state. Its size is consistent with that of a medium sized galaxy.
