The galaxy exhibits a relatively smooth morphology, appearing as a flattened, elongated structure. It is approximately cigar-shaped. The central region displays a yellowish hue, possibly indicating an older stellar population. Fainter blue tinges are visible within the disk, suggestive of more recent star formation. There is no evidence of a strong central bulge, and the disk appears relatively undisturbed, with only slight hints of potential minor disturbances or interactions. No significant tidal features or merging activity are readily apparent.
