This galaxy presents as a relatively compact object with a high degree of central concentration. The overall morphology appears elliptical, exhibiting a smooth light distribution without prominent spiral arms or significant disk-like features. There is a slight elongation visible, but the galaxy is largely spheroidal in shape. The color profile suggests a population of older stars, with a tendency towards redder hues, particularly in the central region. No signs of ongoing major mergers or significant tidal disturbances are apparent, implying a gravitationally relaxed system. The outer regions fade gradually into the background, indicative of a well-defined edge or halo.
