The galaxy appears to be a relatively bright elliptical or lenticular galaxy, exhibiting a smooth, concentrated light profile with minimal visible structure such as spiral arms or distinct dust lanes. The core region appears substantially brighter and more concentrated than the outer regions of the galaxy, exhibiting a yellowish-orange hue, suggestive of an older stellar population with a lower rate of recent star formation. The overall shape is close to round, but appears somewhat elongated in one direction. There is no obvious evidence of a major ongoing merger or significant tidal disturbances.
