The galaxy presents as a spiral type, displaying a prominent disk structure viewed at an angle slightly off from face-on. Two well-defined spiral arms are visible, exhibiting a moderate degree of winding. These arms appear somewhat flocculent, with regions of enhanced brightness suggestive of active star formation. A central bulge is present, exhibiting a moderate size relative to the overall galaxy structure. There is a strong indication of a bar feature traversing the central bulge, which could be influencing the spiral arm structure. No significant morphological disturbances are readily apparent in this image, but the color distribution within the spiral arms suggests that there is likely active star formation. There are no apparent signs of on-going major mergers with neighboring galaxies, though minor interactions cannot be fully excluded.
