The galaxy presents as a centrally concentrated, luminous spheroid. The core region exhibits a high degree of brightness, indicating a substantial concentration of stars. There's a gradual decrease in luminosity as one moves outwards from the center, with a smooth transition towards the outer regions. The galaxy appears largely featureless, lacking prominent spiral arms or significant dust lanes. There may be some slight disturbances in the outer regions but no strong signs of major ongoing mergers or tidal interactions. It is moderately sized, with colors indicating it contains a relatively old stellar population.