The galaxy presents a somewhat irregular morphology. It exhibits a diffuse, faint structure, with hints of a disk-like component. There is evidence of possible disturbances in its form; perhaps minor tidal features or asymmetries in the overall light distribution. The core region appears slightly brighter, though it lacks a pronounced central bulge. Color variations suggest possible variations in stellar populations or dust content across the galaxy, with an indication of bluer colors in some regions compared to others. Overall, this galaxy appears to be a relatively low surface brightness system that may be undergoing or have recently undergone interactions.
