This galaxy appears to be a relatively smooth and centrally concentrated system, likely an elliptical galaxy given its overall morphology. It exhibits a bright core region that gradually fades outwards, showing a radial decline in surface brightness. The shape is slightly elongated. There is little evidence of spiral arms or significant dust lanes. The color profile suggests a population of older stars, as indicated by the reddish hues observed in the image. There might be some subtle distortions hinting at past minor interactions or mergers, however, the overall structure remains largely undisturbed.
