The galaxy appears as a central, luminous spheroid with a smooth light distribution. It presents as generally elliptical. The core region exhibits a concentrated, yellowish-white hue, suggestive of a dominant population of older stars and a lower rate of recent star formation. The outer regions of the galaxy show a gradual decline in brightness, transitioning to a more diffuse, slightly bluer color profile. The structure suggests a lack of prominent spiral arms or a distinct disk component. There is no obvious morphological evidence of recent major merger events or strong tidal disturbances. It is a fairly isolated galaxy.
