The galaxy exhibits a somewhat elliptical morphology with a noticeable central bulge that appears brighter than the surrounding disk. The disk itself presents a mottled texture with indications of spiral arm structures, although these are not sharply defined. Patches of bluer light, suggestive of younger stellar populations and ongoing star formation, are observed within the disk, particularly in the outer regions and potentially along the spiral arms. The overall color of the galaxy trends toward a yellow-white hue, indicating the presence of both older and younger stars. There is a subtle asymmetry in the light distribution, possibly hinting at a minor interaction or tidal disturbance. The edges of the galaxy are somewhat indistinct, fading into the background sky.
