The galaxy presents as a flattened, elliptical morphology. The light distribution appears relatively smooth and centrally concentrated with a bright, prominent bulge. A faint, diffuse disk is observed extending outwards, though lacking defined spiral arm structures. Color gradients suggest an older stellar population dominates. There are no obvious signs of strong star formation, or active galactic nuclei activity, and minimal dust extinction. There is some possible evidence of a minor disturbance in the outer regions. Overall, the galaxy is consistent with a relatively evolved, passive system undergoing little current star formation.
