The galaxy appears to be an elliptical type, exhibiting a generally smooth morphology. The central bulge presents a concentrated, bright region with a yellowish-orange hue. The light gradually fades outward from the center, indicating a lower stellar density in the outer regions. There is a slight elongation or asymmetry. Faint wisps or diffuse features exist, possibly indicating minor disturbances due to interactions or mergers. Overall, the galaxy gives the impression of an older stellar population, with a relatively low rate of current star formation.
