The galaxy presents as a spiral type, showing a disk-like structure but with notable irregularities. The morphology suggests a possible interaction or merger event. A prominent feature is a relatively bright, somewhat elongated central bulge, though its size appears moderate compared to the overall disk. There is evidence of spiral arm structure, but the arms are not well-defined and may be disrupted. The disk displays a clumpy appearance, with variations in surface brightness. The color distribution indicates a mix of stellar populations, with regions of bluer light, potentially indicating recent star formation, interspersed with areas of redder light, likely indicating older stellar populations. There is a slight indication of the galaxy being a barred spiral. The overall appearance suggests an actively evolving system.
