The galaxy presents as a spiral structure with tightly wound arms emanating from a central bulge. The bulge appears prominent and centrally concentrated. The disk is not perfectly face-on, showing a slight inclination, evidenced by the elliptical shape of the galaxy as a whole. Dust lanes are not clearly visible in this image. The spiral arms are relatively smooth in appearance without significant knotty structure, suggesting a lack of intense star formation activity in the arms themselves. There is no obvious evidence of a major ongoing merger or significant tidal distortions. The color distribution suggests a mix of stellar populations, with the central bulge appearing more yellow/orange, which is characteristic of older stars. The arms are bluer, indicating the presence of younger, hotter stars, although the limited resolution makes it difficult to discern any distinct star-forming regions. There is a hint of a bar-like feature in the center.
