The galaxy presents a generally smooth, elliptical morphology. The light distribution appears concentrated towards the center, with a gradual decrease in intensity towards the outer regions. There is a suggestion of a slight elongation, but the overall shape is closer to round than cigar-shaped. The central region displays a yellowish hue, potentially indicating an older stellar population. The outer regions exhibit a bluer tint, suggesting the presence of younger stars. No strong evidence of spiral arms or major disturbances is apparent. Overall, the galaxy appears relatively undisturbed, with a dominant smooth structure.
