The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape approximates a flattened spheroid, displaying a somewhat elongated morphology, but not radically so. The light distribution appears centrally condensed, with a bright core that gradually fades towards the outer regions of the galaxy. The color profile suggests a population of intermediate-age to older stars. There is a hint of subtle internal structure or faint disky feature, but it's predominantly smooth. There is no strong evidence of ongoing mergers or major tidal disturbances, the galaxy appears relatively undisturbed.