The galaxy presents a somewhat irregular morphology. It appears to be a disk galaxy, although the structure is not well-defined. There is a central bulge, but it's not particularly prominent and appears to be of moderate size compared to the rest of the galaxy. Faint spiral arms are likely present, and some signs of disturbance indicate a possible tidal interaction or ongoing minor merger event. The overall color suggests the presence of active star formation, particularly in the disk regions. Dust lanes are not readily apparent but might exist within the fainter areas. The galaxy is neither completely smooth nor clearly indicative of a major merger.
