The galaxy presents a diffuse, somewhat irregular morphology. The central region appears brighter and more concentrated, suggesting a bulge, but it lacks a distinct, well-defined nucleus. There is evidence of extended, fainter features surrounding the central region, possibly indicative of a disk-like structure, although the lack of strong spiral arms or a clear disk plane suggests it may be highly disrupted or irregular. The color distribution appears relatively uniform, with a slightly bluer tint in certain regions. This may indicate ongoing star formation, though at a relatively low rate, or a population of younger, hotter stars. There is the suggestion of a possible tidal tail or faint bridge feature, implying that this galaxy may have experienced, or be experiencing, a gravitational interaction or merger with another galaxy. Overall, the galaxy appears to be a dwarf galaxy that has a disturbed morphology, possibly due to interactions or mergers with other galaxies.
