This galaxy presents as a single, dominant, and relatively smooth elliptical-type galaxy with a concentrated bulge. The light profile appears to be fairly uniform, lacking any strong indication of spiral arms or significant dust lanes. The galaxy exhibits a yellowish-orange hue, which suggests a population of older stars and a dearth of active star formation. The shape appears nearly circular, showing a high degree of rotational symmetry. There is no visual evidence of a major merger event or significant tidal disturbances, with the overall structure appearing relaxed and well-defined. 
