The galaxy presents as a concentrated elliptical, exhibiting a smooth, largely featureless morphology. The core region is characterized by a bright, yellowish-white glow, suggesting a population of older stars. Moving outwards from the core, the color transitions slightly toward a redder hue, implying a shift in stellar populations or dust composition in the outer regions. There are no prominent spiral arms or distinct features indicative of active star formation. The overall shape appears generally rounded, with a slight elongation visible along one axis. There is no visual evidence of tidal tails, mergers, or major disturbances in its structure, suggesting it is a relatively undisturbed system.
