The galaxy presents as a diffuse, relatively faint object. Its overall morphology appears somewhat amorphous, lacking a clearly defined spiral structure or elliptical shape. The light distribution suggests a central concentration, but it is not particularly prominent, indicating a possibly low-luminosity nucleus or a face-on disk orientation. There is a hint of possible tidal features, or perhaps dust lanes, however these are not well defined. The color appears somewhat uniform across the galaxy, indicating a fairly homogenous stellar population. A slight deviation in the morphology, or a potential disturbance, is observed. Overall, the galaxy's appearance suggests it might be undergoing some form of interaction or recent star formation activity, however a significant portion of the light may also be artifacts. 
