The galaxy presents a generally smooth morphology. The object appears elliptical in shape, with a noticeable elongation. The central region exhibits a high concentration of light, suggesting a prominent galactic bulge. The color profile indicates a population of older stars, evidenced by the yellowish-red hue dominating the central region and the overall smooth color gradient, with very little blue light present, suggesting a low rate of on-going star formation. There is no visible evidence of spiral arm structures or significant dust lanes. The smooth features may be undergoing, or have completed, a merger event.
