The galaxy presents as a luminous disk galaxy, viewed at an oblique angle. It exhibits a prominent central bulge that is yellowish-white, suggestive of an older stellar population. A flattened disk surrounds this bulge, with a color gradient transitioning from yellowish-white near the center to a bluer hue further out. This could indicate the presence of younger, hotter stars in the outer regions. The disk appears to be slightly disturbed. There are no readily visible spiral arm structures, and it seems to be smooth. The galaxy appears undisturbed by any major merging events.
