The galaxy presents a disk-like morphology, although the inclination angle obscures a clear view of spiral arm structure, if any exists. A prominent bulge is visible, exhibiting a yellowish-white hue, indicative of an older stellar population and potentially lower star formation activity in this central region. The outer regions of the galaxy are less defined, displaying a bluer tint that likely corresponds to younger, hotter stars within the disk. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions. There may be a faint hint of asymmetry or a minor perturbation in the disk structure, though it is difficult to discern due to the image quality. The overall shape is somewhere between round and cigar-shaped.
