The galaxy presents as a moderately inclined, disk-shaped structure. The central bulge appears prominent, exhibiting a smooth, concentrated distribution of light with a slightly redder hue compared to the outer disk. The disk itself shows evidence of spiral arm structure, although somewhat faint and not sharply defined. These arms exhibit a bluer color, indicative of recent star formation. The galaxy appears relatively undisturbed, showing no strong signs of major mergers or tidal distortions. Overall, the galaxy appears to be a relatively normal spiral galaxy with ongoing star formation, as inferred from the blue color in the spiral arms.
