The galaxy presents as a relatively smooth, elliptical structure. It exhibits a centrally concentrated bulge, appearing bright white, which likely contains older stellar populations. The overall shape leans toward an intermediate ellipticity, not perfectly spherical but also not highly elongated. There's a subtle color gradient, with the central bulge appearing whiter, possibly indicative of a lack of ongoing star formation. Fainter, bluer hues are present in the outer regions, potentially suggesting younger stars. There are no obvious signs of spiral arms, bars, or major disturbances suggesting a merger. The galaxy appears relatively isolated and undisturbed.
