The galaxy presents a disk-like morphology, although it is not perfectly circular. A luminous central bulge is visible, appearing smooth and concentrated. The disk component exhibits a mottled texture, suggesting a spiral structure, albeit somewhat irregular. Some regions of the disk appear bluer in color, potentially indicating areas of active star formation. A less massive, yellowish nearby galaxy appears to be interacting with the primary galaxy, as indicated by the bridge of stars, dust, and gas connecting the two. The galaxy appears to be massive, likely composed of billions of stars. Based on its irregular disk and interaction with a nearby galaxy, it may be undergoing a merging process. The galaxy is also actively forming stars within its disk.
