The galaxy presents as a relatively smooth, centralized light distribution, appearing somewhat elliptical in shape, though nearly circular. The light is most intense at the galactic center, displaying a gradual falloff in brightness towards the outer edges. There is a suggestion of subtle color variation, with the central region exhibiting a warmer, yellower hue compared to the slightly cooler, bluer light in the outer regions. No distinct spiral arms or bar structures are readily discernible. The overall structure appears largely undisturbed, lacking any obvious signs of recent major mergers or significant tidal disruptions. A very slight asymmetry in the outer halo suggests a possible minor interaction, or perhaps internal processes influencing the shape.
