The galaxy presents as a slightly elongated, centrally concentrated object, most likely an elliptical galaxy. The core region exhibits a bright, yellowish-orange hue, suggesting an older stellar population. The outer regions of the galaxy gradually fade into a diffuse halo, which is bluer in coloration than the core, indicating the presence of some younger stars or ongoing, low-level star formation. The galaxy appears relatively undisturbed, lacking any obvious signs of a recent major merger event. There is a slight suggestion of faint spiral arms, but that is not completely obvious. The overall appearance suggests that the galaxy is a massive system with an estimated diameter of 7.5 kpc, exhibiting low but nonzero levels of star formation activity.
