The galaxy presents as a spiral type. The morphology is dominated by a distinct disk structure, with a notable presence of spiral arms. The spiral arms appear tightly wound, indicating a possible grand-design structure. The presence of a bar feature appears to be a possibility within the central region. A bulge is observable, contributing significantly to the central luminosity. The overall color suggests a mix of stellar populations, with a bluer hue associated with star formation regions within the spiral arms. The disk appears relatively undisturbed, showing minimal signs of major merging events.
