The galaxy presents as a generally smooth object with a hint of disk-like structure. It appears moderately rounded. The galaxy exhibits a color gradient, transitioning from a redder hue in the central region to a bluer hue in the outer regions. This color gradient may indicate a radial difference in stellar populations or dust content, with the central region potentially harboring older stars or a higher concentration of dust. There is an indication of some disturbance, possibly tidal interactions or ongoing minor mergers. The galaxy is moderately luminous. The overall morphology suggests an elliptical galaxy or a spiral galaxy with a dominant bulge component.
