The galaxy presents an elliptical morphology, with a smooth, centrally concentrated light distribution. The core exhibits a bright, yellowish hue that fades gradually into a reddish outer halo. Faint, diffuse extensions are visible on either side of the galaxy, suggesting possible tidal interactions or minor disturbances. There is a secondary, smaller and more diffuse galaxy located very close to the primary, brighter one. The interaction may be the cause of the disturbances. The overall color indicates a population dominated by older stars and a relatively low rate of ongoing star formation.
