This galaxy exhibits a pronounced elongated, cigar-like morphology. A central bulge is apparent, displaying a yellowish-orange hue, possibly indicative of an older stellar population and lower star formation rate. Fainter, bluish extensions emanate from the central region, suggesting a disk-like structure with ongoing, albeit subdued, star formation. The smooth appearance dominates, with no major disturbances or prominent spiral arms visible. Overall, the galaxy presents a well-defined structure without evidence of ongoing merging activity, although a small object close to the galaxy could be interacting with it.