The galaxy presents an elongated, cigar-shaped morphology, suggestive of an elliptical galaxy viewed at an angle. The light distribution appears relatively smooth and centrally concentrated with a bright core region. Some subtle features can be discerned, including possible disturbances in the outer regions which may indicate the presence of tidal tails and a merger event in the past. The color suggests an older stellar population dominated by redder stars, consistent with a low star formation rate. Overall, this galaxy appears to be a massive, evolved system, possibly undergoing a morphological transformation.
