The galaxy appears as an elliptical or lenticular type, exhibiting a generally smooth and concentrated central bulge. The overall form is somewhat rounded. There's a subtle hint of a disk-like structure but it is very faint. Star formation appears subdued or largely absent, with a bias toward older stellar populations dominating the color profile. There's no obvious evidence of ongoing mergers or major disturbances in the galaxy's structure. The galaxy is a significant mass, indicative of a mature system that has likely undergone considerable evolution.
