The galaxy presents as an elongated, disk-like structure, consistent with a late-type spiral galaxy viewed at a high inclination angle or potentially a lenticular galaxy. The central region displays a concentration of light, suggesting the presence of a bulge. The galaxy exhibits a smooth texture, with little apparent structure within its disk. There is some variation in color visible across the galaxy, with the central bulge appearing yellower and the outer disk exhibiting bluer hues. The bluer color might be due to the presence of more massive, younger stars associated with on-going or recent star formation in the disk. The overall structure appears relatively undisturbed, without any obvious signs of tidal interactions or mergers.
