The galaxy presents as a disk-shaped morphology, elongated along its major axis, with moderate asymmetry. The central region exhibits a concentrated bulge. The color profile shows a distinct gradient; the core region leans towards redder wavelengths, possibly indicating an older stellar population or dust obscuration. Moving outwards from the core to the disk, the color gradually shifts to bluer wavelengths, hinting at more recent star formation activity within the spiral arms. Patches of star-forming regions are suspected in the blue areas. The disk appears relatively smooth, but might have some irregularities, and there are no strong signs of mergers.
