The galaxy appears as a faint, diffuse object. It presents a flattened, disk-like morphology, though the resolution limitations make a precise determination of spiral arm structure impossible. However, the lack of defined structure in the light distribution and a low level of defined feature suggest the presence of a smooth light profile. A slight colour gradient is observable. It has a noticeable red colour, indicating an older stellar population. There may be a hint of minor disturbances or tidal features, suggesting possible past interactions or ongoing minor mergers, although this is difficult to confirm due to the signal-to-noise ratio of the image. The object is relatively small in angular size. The overall appearance suggests a galaxy with low surface brightness, and there is evidence for it being a relatively old and quiescent system.
