The galaxy presents as a largely featureless, elliptical-like structure. The light distribution appears smooth and concentrated towards the center, suggesting a dominant bulge component. A color gradient is observed, with the core exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. The outer regions display a bluer tinge, possibly indicating younger stars, though this is less pronounced. There is no readily apparent spiral arm structure or dust lane obscuration. The galaxy's overall shape is close to circular, showing only slight elongation. No significant signs of tidal disturbances or mergers are visually evident.