The galaxy exhibits a prominent spiral structure. The spiral arms are tightly wound and somewhat flocculent, appearing as patchy segments rather than continuous, well-defined structures. The central bulge is moderately sized and appears yellowish, indicating a population of older stars. The disk component has a bluer hue, suggesting the presence of younger stars and ongoing star formation. There is no obvious bar structure visible in the image, though there is a slight elongation that could be indicative of a weak bar. There are no signs of major mergers or significant tidal disturbances, though there is a slight asymmetry. Overall, the galaxy seems to be a relatively undisturbed spiral galaxy with a moderately active rate of star formation.
