The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, concentrated light distribution. The central region displays a yellowish hue, potentially indicating an older stellar population and a relative lack of ongoing star formation. There is a faint, extended halo surrounding the core, appearing somewhat elongated. No distinct spiral arms or prominent dust lanes are discernible. There are slight signs of a minor merger or tidal disturbance. The galaxy appears to be relatively isolated, with no nearby companions visibly interacting with it.
