The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated, bright central bulge that fades gradually into the outer regions. The color profile suggests an older stellar population, with a redder hue dominating the inner regions. There may be hints of spiral structure, although they are faint and lack definition. The overall morphology appears undisturbed, showing no obvious signs of tidal interactions or major mergers. The galaxy appears to be relatively isolated.
