The galaxy presents as an edge-on spiral. It exhibits a prominent central bulge that appears somewhat elongated. The bulge displays a yellowish-orange hue, potentially indicative of an older stellar population. The disk is visibly thin and elongated, characterized by a bluish tint. This suggests the presence of younger, hotter stars and ongoing star formation within the disk. There appears to be a slight warping or asymmetry visible in the disk. No obvious dust lanes are readily apparent in the image, though some obscuration may be present closer to the central bulge. Overall, the galaxy appears relatively undisturbed, with no signs of major merging activity.
