The galaxy presents as a spiral type, viewed at a significant angle relative to our line of sight, appearing close to edge-on. A central bulge is discernible but not dominant, appearing moderately sized relative to the disk. The galaxy exhibits a well-defined disk structure. The presence of spiral arms is strongly suggested, though their morphology is difficult to discern due to the angle of observation. There is no strong evidence of a bar structure crossing the bulge, and the disk appears relatively undisturbed. The overall color is a gradient, shifting from a yellowish hue at its central region, indicative of older stellar populations, to a bluer hue at the outer edges, suggesting the presence of younger stars and ongoing star formation. The disk is noticeably warped or flared, and there is minimal to no evidence of recent major mergers or strong tidal disturbances.
