The galaxy presents as a relatively smooth, elliptical morphology. There is a high degree of central concentration, with the light intensity decreasing gradually outwards. The galaxy exhibits a generally round shape but has an inclination that gives it a slightly elongated appearance. There is little evidence of distinct spiral arms, or strong dust lanes. The galaxy's color gradient suggests a population of older stars, with a slight reddening towards the core. There is no immediately apparent evidence of ongoing major mergers or significant tidal disturbances, although a minor interaction cannot be ruled out.
