The galaxy presents as a somewhat rounded, centrally concentrated object. A smooth light distribution dominates, indicating an elliptical morphology or potentially a face-on spiral with a prominent bulge and tightly wound arms that are not resolvable at this resolution. Color gradients are subtle, although the central region appears slightly redder than the outer regions. There is no definitive evidence of spiral arms or a bar structure. The galaxy does not appear to be undergoing a major merger, but the possibility of minor disturbances within the galaxy cannot be ruled out, as indicated by the slight asymmetry in its light distribution. The estimated size indicates a relatively compact galaxy. Overall, the galaxy is a fairly regular and quiescent system.
