The galaxy appears to be a spiral galaxy, viewed at an oblique angle, with the galactic disk tilted relative to our line of sight. The central bulge exhibits a concentrated, relatively smooth light profile, appearing somewhat spheroidal. Faint spiral arm structures are suggested by subtle color variations within the disk, extending outwards from the central bulge. The overall color distribution indicates a mix of stellar populations, with the bulge appearing bluer and the outer disk regions appearing redder, possibly indicating ongoing star formation or dust absorption. There appears to be a slight distortion and tidal disturbances, possibly due to a past or ongoing minor merger event. Some faint red patches indicate HII regions or areas of intense star formation. Overall, the galaxy appears to be a late-type spiral galaxy undergoing active, but not extreme, star formation.
