The galaxy presents a generally smooth morphology, with a structure that appears to be between round and elongated. It exhibits a color gradient, transitioning from a yellowish core to a bluer outer halo. There appears to be some minor distortions or irregularities in the overall form, possibly indicating an interaction with another galaxy or internal disturbances. The light distribution is concentrated towards the center, suggesting a higher density of older stars there, with a gradual decline in luminosity towards the outer edges.
