The galaxy presents a largely smooth morphology with little to no discernible spiral arm structure. The core appears bright and concentrated with a yellow-white hue, suggesting a significant population of older stars. The galaxy exhibits a slight ellipticity, appearing more elongated than perfectly circular, trending more to a cigar shape. Faint extensions of diffuse light are visible extending outwards from the central region, indicating a gradual decrease in stellar density with increasing radius. There is a subtle hint of disk-like structure that is causing the deviation in roundness from the core to the extent of the halo. There are no obvious signs of ongoing major mergers or significant tidal disturbances in the visible light.
