The galaxy appears as a moderately sized, elliptical-like structure. It presents a smooth, generally featureless profile. The core is yellowish and relatively bright, indicating an older stellar population or dust concentration. The outer regions are fainter and exhibit a slightly bluer hue compared to the core, which could represent a younger stellar population in those areas. No prominent spiral arms or distinct features are visible. The overall shape is somewhat round, with a slight deviation from perfect circularity. There is no evidence of ongoing major mergers or significant tidal disturbances.
