The galaxy presents as a concentrated spheroid, exhibiting a dominant central bulge. It displays a smooth, relatively featureless morphology, lacking prominent spiral arms or irregular structures. The light distribution appears centrally concentrated with a gradual decrease in intensity towards the outer regions. Color gradients suggest a population of older stars, with the core exhibiting a reddish-yellow hue. There may be some minor disturbances visible which could be due to tidal interactions. No distinct dust lanes are visible.
