The galaxy displays a clear spiral structure. It appears to be a face-on or nearly face-on spiral galaxy with a prominent central bulge. The spiral arms are loosely wound, extending outwards from the bulge. There appears to be evidence of a bar structure bisecting the central bulge. The arms show some degree of patchiness, possibly indicative of star-forming regions within the spiral arms. The galaxy's overall color suggests a mix of stellar populations, with the bulge appearing yellower, likely due to older stars, and the arms showing bluer hues, potentially indicating the presence of younger, hotter stars. There is no obvious indication of major mergers or significant tidal disturbances.
