The galaxy presents as a somewhat face-on spiral, possibly an intermediate type, although the disk structure is not highly pronounced. There's a noticeable central bulge that appears yellowish, suggesting an older stellar population. The spiral arms are loosely wound and exhibit a bluish tint, indicative of ongoing star formation. The overall color of the galaxy appears to be slightly redder, potentially due to dust obscuration or an older stellar population compared to typical spiral galaxies. The galaxy appears to be relatively undisturbed, without any major signs of mergers or tidal distortions.
