The galaxy presents a generally smooth morphology, with a high degree of central concentration. It appears elliptical in shape, with an axial ratio suggesting a classification between round and cigar-shaped. The central region exhibits a bright, concentrated luminosity profile. The overall color is consistent with an older stellar population, with redder hues dominating. There are subtle features indicating a possible disk component and/or minor disturbances, however, these are not immediately apparent. There is no evidence of a major merger or significant tidal disruption. The galaxy appears to be a relatively undisturbed system.
