The galaxy presents as a spiral type, observed nearly face-on. Its overall structure exhibits a distinct central bulge, characterized by a yellowish hue, which suggests a population of older stars. Surrounding the bulge, the galactic disk displays prominent spiral arms. These arms appear tightly wound, originating close to the bulge and extending outwards. A degree of patchiness along the arms suggests active star formation regions.

The galactic disk displays a blueish tint, indicating the presence of younger, hotter stars, as expected in a spiral galaxy with ongoing star formation. There appears to be a weak or no bar structure within the central region. There is a smooth transition in color from the center to the outer edges of the spiral arms, but there is no evidence of major disturbances or ongoing mergers.
