The galaxy presents as a relatively smooth, elliptical structure with a bright, concentrated central bulge. The morphology appears largely undisturbed, with no obvious signs of ongoing major mergers or significant tidal interactions. There is a slight hint of a flattened disk-like structure. The galaxy exhibits a color gradient, transitioning from a yellowish-orange core to a subtly greenish-blue hue in the outer regions. The overall color suggests a stellar population dominated by older stars with a possible presence of younger stars in the disk region. Star formation activity is likely to be relatively low.
