The galaxy appears to be a relatively compact, elliptical type. The light profile is centrally concentrated with a smooth, diffuse halo extending outwards. The core exhibits a yellowish hue, potentially indicative of an older stellar population. There is a faint, extended outer envelope that is almost round. The galaxy does not show any obvious signs of spiral arm structures or significant dust lanes. There are no clear signs of active star formation regions. Overall, this galaxy presents as a relaxed, evolved system.
