This galaxy presents a generally smooth and elliptical morphology. Its light is concentrated in the center, with a gradual decrease in intensity outwards, creating a diffuse halo. The galaxy appears largely featureless, without any obvious spiral arm structures or significant dust lanes. Its color profile indicates a redder overall population, potentially indicating a higher proportion of older stars and a relatively lower rate of ongoing star formation. There are no visible signs of a major ongoing merger, although minor disturbances cannot be ruled out based on this image alone. The galaxy's shape is observed to be mostly round, without a pronounced elongated appearance. Overall, it appears to be a mature and well-defined system.
