The galaxy presents as a centrally concentrated luminous object with a roughly elliptical morphology. The color profile suggests a population of older stars, with a yellow-red hue dominating the central region and extending outwards. A bluer component is faintly visible in the outer regions of the disk. The galaxy appears relatively undisturbed with a high degree of central smoothness and no obvious signs of spiral arms or major mergers. There may be minor disturbances indicating smaller mergers. The shape ranges between round and cigar-shaped. The galaxy exhibits no strong evidence of significant ongoing star formation.
