Observed galaxy presents a primarily smooth morphology. There is evidence of a central bulge with a gradual decrease in luminosity outward. Color gradients suggest an older stellar population concentrated in the central region, appearing yellower, with hints of bluer components in the outer regions, suggesting younger stars or regions of ongoing star formation, although these features are subtle. There are no distinct spiral arms or a well-defined disk structure visible. Subtle indications of tidal disturbances are visible in the form of faint, asymmetric extensions. The main body of the galaxy is centrally concentrated, displaying a relatively elliptical shape, appearing to be relatively compact. Evidence suggests the possibility of a minor merger or tidal interaction, indicating a possible disturbance of its structure.
