The galaxy presents a generally disk-like morphology, albeit with notable irregularities. The central region appears as a bright, concentrated bulge, possibly indicating an older stellar population. Extending outwards from the bulge is a fainter, elongated disk. Within the disk, there are indications of spiral arm structures, though they are not sharply defined. A clumpy appearance to the disk hints at ongoing star formation regions or dust obscuration. Evident are what appear to be a few bright, localized areas of intense emission, primarily in the redder wavelengths. These areas are likely HII regions, indicative of active star formation. Overall, the galaxy presents a morphology consistent with a spiral galaxy undergoing active star formation, along with potential signs of a minor disturbance due to a possible recent or ongoing interaction with a smaller galaxy, most visible on the left side of the galaxy.
