The galaxy exhibits a complex morphology, characterized by a disturbed structure. There is a faint disk-like component. The central region appears diffuse, with no distinct nucleus visible. There are asymmetries, and the overall form suggests a galaxy that may be undergoing a merging event or exhibiting tidal disturbances. Color gradients are subtle, primarily redder towards the fainter, outer regions and bluer in small areas, hinting at regions of ongoing star formation activity. Faint extensions or tidal tails might be present, extending outwards from the main body, though their presence is uncertain due to the image quality. Overall, the galaxy is relatively faint and small, based on its approximate size and magnitude, and presents with significant morphological irregularities.
