The galaxy presents as a somewhat faint, diffuse object of moderate angular size. Its overall morphology appears irregular, with a somewhat elongated shape and a lack of well-defined spiral arms or a prominent central bulge. The light distribution within the galaxy seems uneven, indicating variations in stellar density and/or dust obscuration. There appears to be a possible tidal tail, which could point to a previous or ongoing gravitational interaction. It is also possible that there are some minor disturbances apparent. The color of the galaxy is generally consistent, with a slight shift toward redder hues, which would imply an older stellar population. 
