The galaxy appears as a single, concentrated, unresolved object. It exhibits a generally smooth morphology, with no obvious spiral arm structures or prominent dust lanes visible. The color profile is relatively uniform, with a subtle transition from a warmer, yellower central region to a slightly cooler, bluer outer halo. The overall shape approximates a rounded structure with a possible slight elongation. There is no indication of any major mergers or significant tidal disturbances. The galaxy likely represents a large mass system undergoing active star formation, but not at an extreme rate.
