The galaxy presents as a singular, mostly homogenous entity. It exhibits a generally elliptical morphology and appears to be substantially smooth in texture, with little to no discernible substructure such as spiral arms or bar features. The color profile tends towards the redder end of the spectrum. The galaxy shows negligible evidence of tidal disturbances or ongoing mergers. The apparent uniform color and lack of distinct features suggest a stellar population that is primarily older, with limited ongoing star formation. Its compact appearance suggests that the light emitted is concentrated in a relatively small area.
