The galaxy appears to be a relatively smooth, elliptical galaxy, though not perfectly round. It displays a concentration of light towards its center, suggesting a prominent bulge. The galaxy is subtly elongated with no clear evidence of spiral arms or a distinct disk structure. There might be a slight asymmetry, possibly indicating a minor disturbance or interaction, although no significant merging or major disruption is readily apparent. The color gradient suggests an older stellar population, with a reddish hue. Star formation seems to be occurring at a slow rate.
