The galaxy presents an elongated, cigar-like morphology with a relatively smooth appearance. The central region exhibits a concentration of light, suggesting the presence of a bulge, potentially indicating an older stellar population. Extending outward from the bulge is a disk structure. The disk displays a subtle blueish tint, implying recent or ongoing star formation, although not intensely so. There appears to be little to no evidence of spiral arm structure, or bars. There are some indications of minor disturbances. Based on these observed features, the galaxy is likely an early to intermediate type spiral galaxy, perhaps similar to an edge-on lenticular galaxy.
