The galaxy presents as a spiral type, exhibiting a disk structure with visible spiral arms. While the spiral arms are discernable, the morphology suggests they are not tightly wound. A prominent central bulge is observed, approximately moderate in size compared to the overall disk. The galaxy displays an overall bluish hue, indicative of ongoing star formation. There is no strong evidence of a bar feature bisecting the bulge. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The edges of the galaxy appear smooth.