The galaxy presents as a relatively smooth, elliptical structure. The core exhibits a concentrated, bright region. Moving outward, the galaxy fades into a more diffuse halo. While generally rounded, there is a slight elongation present in its overall shape. There is no obvious spiral arm structure or significant dust lane features. The galaxy appears to be relatively undisturbed, showing no strong signs of a recent major merger event. Color gradients suggest that the central region contains an older stellar population relative to the outer regions, which appear bluer. There is a subtle irregularity in the extended halo, hinting at a potential minor interaction or past accretion event.
