The galaxy presents a generally smooth, elliptical morphology, elongated in shape. The central region exhibits a high concentration of light, suggestive of a substantial bulge component. A faint disk-like structure is suspected, although definitive features like spiral arms are not visible in this image. There is a slight asymmetry in the outer regions, suggesting a possible minor gravitational interaction or past merger event. The color profile suggests a population of older stars, as evidenced by the reddish hues, with only a subtle hint of blue light possibly indicating a low level of ongoing star formation. Overall, the galaxy appears to be relatively evolved and quiescent.
