The galaxy presents as a relatively face-on spiral with a prominent central bulge exhibiting a yellow hue, likely indicating an older stellar population. Faint spiral arms are discernible, exhibiting a bluer tint suggestive of more recent star formation. The spiral structure appears somewhat flocculent, with patchy areas of star formation rather than well-defined, continuous arms. There may be some minor distortions in the disk, potentially indicating past or ongoing interactions. Overall, the galaxy displays characteristics of a massive system with ongoing, though potentially subdued, star formation.
