The galaxy appears to be a spiral galaxy viewed at a slight angle. It exhibits a central bulge region that presents a reddish-orange hue, possibly indicating an older stellar population with less active star formation. A faint disk structure surrounds the bulge. This disk shows evidence of spiral arms, with a subtle bluish tint, suggesting the presence of younger, hotter stars and ongoing star formation within these arms. The arms are not sharply defined, giving the galaxy a somewhat flocculent appearance. Overall, the galaxy displays a moderate level of internal structure without any signs of major mergers or tidal disturbances. The disk of the galaxy appears smooth and relatively undisturbed, with a small fraction of the galaxy light distributed in a diffuse halo surrounding the main body.
