The galaxy appears to be a spiral type, exhibiting a disk structure with prominent spiral arms. There is evidence of a central bulge, though it appears relatively small compared to the overall disk size. The spiral arms show a somewhat tightly wound morphology. The color distribution suggests ongoing star formation activity within the spiral arms, as indicated by a bluish hue. The dust lanes can be seen along the inner edges of some of the spiral arms. There may be signs of some tidal features or minor distortions, but a major merger event is unlikely based on the overall structure. The object is seen face-on. There may be a bar structure present, though it is difficult to resolve due to image quality.