The galaxy presents as a centrally concentrated object with a relatively smooth morphology. The galaxy exhibits a discernible color gradient, with a yellowish-white core transitioning to a bluer, diffuse outer region. The light distribution appears to be moderately elliptical, suggesting a flattened spheroidal or disk-like structure viewed at an angle. There are faint hints of asymmetry in the outer regions, possibly indicating minor tidal disturbances or interactions. Overall, the galaxy appears to be a moderately massive system with ongoing, but not intensely rapid, star formation.