The galaxy presents as a somewhat elliptical, disk-like structure. The central bulge appears bright and concentrated, exhibiting a yellowish-white hue. The surrounding disk shows a gradual decrease in luminosity extending outwards from the core. The disk also shows some blue, suggesting some active star formation. There is no significant evidence of spiral arm structures within this visible image. The smooth appearance of the galaxy indicates it is likely a relatively evolved system. There are no readily apparent signs of ongoing major mergers or tidal disturbances. It appears to be a well-defined and relatively isolated galaxy.
