The galaxy presents as a generally smooth, elliptical-like structure with a concentrated central bulge. There appears to be little to no evidence of spiral arm structure. The galaxy exhibits a radial color gradient, transitioning from a yellow/orange hue in the core to a bluer color in the outer regions. This may indicate differing stellar populations or dust distributions. No major disturbances are apparent within the galaxy’s morphology. The overall shape appears relatively round and undisturbed. The galaxy appears to be a single, isolated entity.
