The galaxy presents as a centrally concentrated object with a smooth and largely featureless morphology. It exhibits a generally elliptical shape, appearing highly rounded. The color profile suggests a dominant population of older stars, indicated by the reddish-yellow hue concentrated towards the core, which gradually transitions to a bluer tint in the outer regions. There is no apparent evidence of spiral arms, a bar structure, or significant dust lanes. The galaxy displays no clear signs of ongoing or recent major mergers or tidal disturbances, suggesting a relatively quiescent state.
