The galaxy presents as an edge-on spiral or lenticular galaxy, exhibiting a flattened, disk-like structure. There is a noticeable central bulge, appearing brighter and more concentrated than the surrounding disk. The disk itself shows a relatively smooth texture, with minimal visible dust lanes or distinct spiral arm structures, although there may be the beginning of some spiral structure. The overall color appears to be more towards the red end of the spectrum, which could indicate an older stellar population with a low ongoing star formation rate, and a high amount of dust obscuring the younger bluer stars. The galaxy seems to be relatively undisturbed, showing no obvious signs of a major merger or tidal interactions. The outer regions of the disk fade gradually into the background sky, indicating a lack of a sharp cutoff. The object has an estimated size of ~6 kpc.
