This galaxy exhibits a clear spiral structure with prominent arms. These arms appear loosely wound and extend outwards from a central bulge. The bulge itself appears to be of moderate size and shows a yellow-orange hue, suggesting a population of older stars. The spiral arms are bluer in color, indicating the presence of younger, hotter stars and active star formation regions. The morphology appears disturbed, possibly due to a minor interaction or ongoing merger, showing an asymmetrical structure within the arms. It is likely a relatively massive galaxy, with moderate ongoing star formation. Bar feature is also apparent across the bulge.
