This galaxy appears to be a spiral galaxy, observed at a slight angle to face-on. A central bulge of older stars exhibiting a yellowish hue dominates the core. Fainter spiral arms extend outwards, showing hints of blue, suggesting ongoing star formation. The galaxy is not perfectly symmetrical, with a subtle asymmetry in the arm structure, which could be indicative of past or ongoing minor interactions. There are no signs of major mergers or tidal tails visible in this image. The disk of the galaxy appears relatively smooth, without pronounced knots of star formation or dust lanes easily discernible at this resolution. The overall structure suggests an intermediate-mass galaxy with a moderate star formation rate.
