The galaxy presents as a generally smooth object, exhibiting an elliptical morphology. It displays a concentrated central bulge, with light diminishing gradually towards the outer edges. The shape appears to be more in-between round and elongated. There is no strong evidence of spiral arm structure or significant star formation regions visible in this image. The color profile suggests a population of older stars, particularly in the central region, and a comparatively lower proportion of younger, bluer stars throughout the galaxy. No signs of major disturbances or mergers are immediately apparent.