The galaxy presents as a fairly compact and luminous object. It exhibits a central, concentrated bulge that dominates its overall morphology. The color gradient suggests a higher concentration of older stellar populations within the central bulge, indicated by its yellowish-red hue. Fainter, bluer extensions surround the core, potentially representing a more recent period of star formation activity at larger radii. No distinct spiral arms are apparent. The galaxy has a mostly smooth appearance, with a slight degree of ellipticity. There are no obvious signs of ongoing major mergers or significant tidal disturbances affecting its structure.
