The galaxy presents as a centrally concentrated, smooth object with an elliptical morphology. It exhibits a dominant, bright central bulge that fades gradually toward its outer edges. The core region is characterized by a yellowish hue, suggesting an older stellar population. The outer regions appear slightly redder, indicating the presence of dust or potentially older, cooler stars. There is no clear evidence of spiral arms or significant substructure within the galaxy. The overall appearance is consistent with an early-type galaxy, possibly an elliptical galaxy or a lenticular galaxy viewed close to face-on. There are no visible signs of ongoing major merging activity or strong tidal disturbances; however, there may be a slight asymmetry that implies a past minor disturbance.
