This galaxy presents as a relatively compact, round object with a smooth, almost spheroidal morphology. There are indications of a central bulge dominating the structure. The galaxy exhibits a color gradient, appearing bluer towards the central region and becoming redder in the outer parts. This suggests that star formation activity is concentrated in the core, with an older stellar population in the outskirts. There is no obvious spiral arm structure or prominent dust lanes visible. Minor disturbances could be present but are not readily apparent. The lack of strong tidal features suggests that this object has not recently undergone a major merger.
