The galaxy appears to be a spiral type, with a disk-like structure readily apparent. The orientation is nearly edge-on, presenting a flattened profile. Two prominent spiral arms are distinctly visible, tracing a wide, open pattern. There is a moderate central bulge. The bulge's color seems somewhat yellower than the disk, possibly indicating an older stellar population. Within the spiral arms, there are regions of bluer light, which could point to more recent star formation. There is no indication of a bar structure. The overall structure seems relatively undisturbed, without significant signs of ongoing major merging activity. The galaxy exhibits a moderate level of internal organization.