The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing largely rounded with a slight elongation. There is a luminous core transitioning into a more diffuse halo. The color profile suggests a population dominated by older stars, based on the redder hues, especially in the central region. There is little evidence of spiral arm structure or significant dust lanes. The overall appearance is consistent with that of an early-type galaxy. There are no obvious signs of major mergers or strong tidal disturbances. Some minor irregularities are seen in the outer halo, but these are minimal and not particularly significant.
