The object presents as an elongated, disk-shaped galaxy, observed at an oblique angle. The central region exhibits a concentrated luminosity, appearing yellowish-orange in color, suggestive of an older stellar population. Progressing outwards, the galaxy displays a distinct, bluish-white hue particularly at the extreme edges. The overall structure appears relatively undisturbed, showing no obvious signs of major mergers or tidal disruptions, although there appears to be some minor disturbances. It can be inferred that this galaxy is undergoing some degree of star formation within its disk regions, which can be inferred from the blue color, but star formation in the core is largely completed. The primary axis of the galaxy is significantly longer than the minor axis, reinforcing the observed elongated or cigar-shaped morphology.
