The galaxy presents as a spiral, with a substantial disk component. Two spiral arms are visible, exhibiting a medium degree of winding. The central bulge is of moderate size, exhibiting a yellow hue. There is no indication of a strong bar structure; instead, the central region shows a more diffuse distribution of light. The galaxy is not observed edge-on. The galaxy is a bluish hue. It shows minor disturbances to its structure, but no clear evidence of an ongoing major merger. The light from the galaxy exhibits a redshift, indicating considerable distance. It has a bright magnitude and a relatively high mass. The rate of star formation is moderate.
