The galaxy presents as a spiral, viewed at a moderate angle. It exhibits a discernible disk structure with evidence of spiral arms, though the arm definition is somewhat diffuse and lacks sharp boundaries. Two arms are clearly visible.

A central bulge is present, appearing relatively small in proportion to the overall disk size. The bulge exhibits a yellowish hue, suggesting a population of older, redder stars. The disk shows a mix of colors, with bluish regions indicating areas of more recent star formation and concentrations of younger, hotter stars. There are no obvious signs of major mergers or significant tidal disturbances. The overall structure appears relatively undisturbed.
