The galaxy presents a morphology that is predominantly smooth and elliptical in appearance. It exhibits a slightly elongated shape, though it is mostly rounded. Its central region is more luminous, with a gradual decrease in intensity towards the outer edges, implying a concentrated distribution of stars. The galaxy displays a relatively simple structure, devoid of prominent spiral arms or significant dust lanes. The color profile suggests a population of older stars. There is no significant evidence of ongoing major merger activity, although some minor irregularities in the outer regions could potentially indicate past or ongoing tidal interactions or minor disturbances.
