This galaxy presents a somewhat irregular morphology. It exhibits a central, brighter region that could represent the galactic bulge, which appears elongated rather than perfectly spherical. There is evidence of a disk-like structure extending outwards from this central region, though the disk is not sharply defined. Some areas of blueish hue within the disk suggest the presence of younger star populations and ongoing star formation. The overall structure hints at the possibility of recent or ongoing interactions, potentially minor disturbances. There isn't clear evidence of a major merger, but the slightly distorted shape lends to this hypothesis. The galaxy does not exhibit a completely smooth appearance.
