The galaxy presents as a somewhat smooth, elliptical or lenticular system with a notable lack of distinct spiral arm structure. It exhibits a concentrated central bulge that graduates outwards, with a moderately round shape. The galaxy displays a color gradient, shifting from a reddish-yellow core to a more blue-white outer region. This color difference suggests a range of stellar populations, with older, redder stars concentrated towards the center and bluer, younger stars distributed within the disc. There appear to be minor irregularities in the shape. No major mergers are evident, but the morphology suggests possible tidal interactions or minor disturbances. The relatively smooth structure and color profile are consistent with a relatively low specific star formation rate and a high stellar mass. 
