The galaxy presents as a relatively smooth, elliptical structure. It exhibits a centrally concentrated brightness profile, with the light intensity gradually decreasing towards the outer regions. The overall shape appears close to circular, with minimal deviation from a round morphology. There are no immediately discernible spiral arms or a prominent disk-like structure. The color distribution indicates a generally older stellar population, with a yellowish-white core that likely consists of older, lower-mass stars. Faint bluish hues are also present, possibly indicating regions of more recent, albeit subdued, star formation activity. There is no strong evidence of ongoing or recent major merger events, though subtle irregularities in the outer halo could suggest minor gravitational interactions in the past. Overall, this galaxy seems to be a relatively isolated elliptical, potentially in a quiescent phase of its evolution.
