The galaxy appears to be relatively small, with a possible, though not distinct, disk structure. The central region is bright and concentrated, possibly indicating a bulge or active galactic nucleus. There is indication of significant disturbance to the structure. Faint tidal features or extended arms may be present, suggesting a potential interaction or past merger event. Overall the galaxy appears to have a distorted morphology with clumpy areas, a central bright region, and a hint of underlying spiral structure that may be in the process of being disrupted. The color profile suggests it may be actively forming stars, and some dust obscuration may be occurring near its core.
