This galaxy appears to be a relatively smooth, elliptical galaxy. It presents a moderately elongated shape, neither perfectly spherical nor highly flattened. The galaxy exhibits a concentrated central bulge that gradually fades into the outer regions. There is no clear evidence of spiral arms or a prominent disk structure. The color profile suggests a population of older stars, with the central bulge appearing somewhat yellower compared to the bluer, fainter outskirts. No signs of recent major mergers or strong tidal disturbances are apparent in the image, though the suggestion of a minor perturbation cannot be excluded based on this image. Overall, the galaxy's morphology indicates it is likely a mature system that has undergone significant stellar evolution, with a relatively low rate of ongoing star formation.
