The galaxy presents a distinct spiral structure, with tightly wound arms emanating from a prominent central bulge. The bulge appears to be of moderate size relative to the overall galactic disk. While the spiral arms are clearly discernible, they exhibit some fuzziness, suggesting ongoing star formation activity within these regions. No strong bar feature is immediately apparent, and the overall galactic structure appears relatively undisturbed, showing no obvious signs of recent major merger events, though there may be some minor distortions. The color distribution indicates a mix of stellar populations, with the bulge potentially harboring older, redder stars, and the spiral arms exhibiting bluer hues indicative of younger stars. The galaxy is not seen edge-on, but rather at an angle where the spiral structure is easily visible.
