The galaxy presents as a well-defined, centrally concentrated object, exhibiting a smooth light distribution. It appears elliptical in shape, with no obvious spiral arm structures or significant dust lanes visible. The color profile indicates a relatively red object, potentially indicative of an older stellar population or a significant amount of dust obscuration, with a slightly yellowish core. The galaxy appears to be relatively undisturbed, showing no obvious signs of a major ongoing merger event, although there may be some minor irregularities in its outer isophotes. Overall, this galaxy appears to be a mature system, likely a massive elliptical galaxy at a moderate redshift.
