The galaxy presents as a spiral with moderately wound arms. A bright central bulge is apparent, with the majority of the galaxy's light concentrated there. The disk appears somewhat inclined relative to our line of sight. Faint spiral arm structures are visible, with a suggestion of fragmentation or flocculence. A slight asymmetry is present in the disk's morphology. The spiral arms appear to have multiple arm segments branching out with a relatively small pitch angle and a low arm to arm angle. The color suggests ongoing star formation within the spiral arms. The overall structure seems relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The observed color distribution indicates a radial gradient, with the central region being redder than the outer spiral arms.
