The galaxy presents as a moderately bright, elliptical or lenticular structure. Its overall shape appears fairly smooth, with a slight elongation. The core exhibits a higher surface brightness, gradually decreasing outwards. There is a suggestion of a weak disk component that is nearly edge on with a bulge in the center. Color gradients suggest a slightly bluer central region, possibly indicative of ongoing star formation. The outer regions appear redder, consistent with an older stellar population. No distinct spiral arm structures or significant dust lanes are visible in this image. There is some slight indication of a disturbance in the galaxy structure, which could be due to a minor merger or a tidal interaction with another galaxy.
