The galaxy exhibits a clear spiral structure, with tightly wound arms emanating from a central bulge. The bulge appears relatively small compared to the overall disk size. The spiral arms display a mottled texture, suggesting areas of active star formation interspersed with regions of lower stellar density. There is evidence of a bar-like structure extending through the central region of the galaxy, oriented roughly horizontally in the image. The color profile indicates a mix of stellar populations, with bluer hues concentrated along the spiral arms, consistent with younger, hotter stars. The disk is viewed at a near face-on angle, allowing for detailed observation of the spiral structure. Overall, the galaxy presents as a well-formed spiral galaxy with ongoing star formation activity. Indications of minor disturbances may be present with some warping on the edges of the spiral arms.
