The galaxy presents a primarily elliptical morphology, exhibiting a smooth, concentrated light profile. The central region appears bright and yellowish, suggesting an older stellar population. The galaxy's overall shape is closer to round, though not perfectly so. There's a lack of distinct spiral arms or prominent dust lanes, and it does not appear to be undergoing any major mergers or significant tidal disturbances. The outer regions show a gradual decrease in luminosity. The color gradient implies a possible change in stellar population from the center outwards, though this is not very pronounced.
