The galaxy presents as a relatively smooth, centrally concentrated structure. It exhibits a predominantly elliptical morphology, appearing largely spheroidal with minimal discernible disk-like features. The color profile suggests a population of older stars, indicated by the reddish-yellow hue dominating the central regions. There is some irregularity in the galaxy structure, possibly indicating minor tidal disturbances, a recent merger, or it could just be internal irregularities. There is no clear evidence of strong spiral arms.