The galaxy presents as a relatively compact and well-defined object. It appears elliptical in shape, exhibiting a smooth light distribution, and appears to lack spiral arms. Its color suggests an older stellar population, with a dominant redder hue and a subtle contribution from younger, bluer stars, possibly hinting at ongoing but low-level star formation within the galaxy. There is some evidence of possible minor disturbances present, either from a past merger event or an ongoing interaction. Based on the morphology, it could be classified as an early-type galaxy, likely an elliptical galaxy.
