The galaxy appears as an elliptical, or possibly lenticular, system. It presents a smooth, diffuse light profile, lacking prominent spiral arms or distinct star-forming regions. The color gradient suggests a centrally concentrated, older stellar population. The object exhibits an elongated shape, appearing cigar-shaped, with the major axis significantly larger than the minor axis. There is no visual evidence of ongoing mergers or major disturbances in its morphology, though the possibility of minor tidal interactions cannot be entirely ruled out based on this single image. The galaxy appears to be a relatively massive system, given its brightness and size.
