The galaxy appears to be a spiral type, exhibiting a distinct disk structure. The spiral arms are tightly wound around a moderately sized central bulge. There may be a slight bar structure. The arms are somewhat difficult to distinguish due to their tight winding, but there seem to be approximately three of them. The disk of the galaxy appears relatively undisturbed, with no signs of a major merger event, though minor disturbances cannot be ruled out. The galaxy does not seem to be edge-on, as the disk is clearly visible. The galaxy's color suggests ongoing star formation, particularly in the disk and spiral arms. The central bulge appears more yellow.