The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is minimal evidence of spiral arms or other disk-like features. The galaxy exhibits a color gradient, appearing yellowish-white towards its center, suggesting a population of older stars, with the color shifting slightly redder towards the outer regions, which could be indicative of a relatively low rate of current star formation. The overall morphology suggests a fairly evolved system that has likely undergone significant merging activity in its past. There is no obvious tidal debris or signs of ongoing major interactions. The shape appears close to circular. There is some possibility of slight disturbances.
