The galaxy presents a distinct disk-like morphology, although not perfectly edge-on. The central bulge is noticeable, displaying a yellow hue indicative of an older stellar population. Fainter, bluish regions are observed within the disk, suggestive of ongoing star formation. The overall structure appears relatively undisturbed, showing no strong evidence of a major merger event, though minor disturbances cannot be ruled out. The galaxy exhibits a moderate degree of star formation activity and a substantial stellar mass. The light distribution from the galactic center outwards suggests a centrally concentrated mass profile.
