The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core region exhibits a yellowish-white hue, which could be indicative of an older stellar population dominating the light emission in that area, with relatively low levels of ongoing star formation. Extending outward from the core, there is a more diffuse halo. The overall shape appears to be mostly round. A region of redder light is visible on one side of the galaxy, possibly indicating a region of dust extinction or a distinct stellar population. There is no clear indication of spiral arms. There may be a very minor disturbance visible, such as a tidal tail.
