The galaxy presents as a spiral, observed at a tilted angle relative to our line of sight. A central bulge is visible, appearing yellowish in color, suggesting an older stellar population concentrated towards the galactic center. The disk exhibits spiral arm structures. These spiral arms are tightly wound and display a bluer hue, indicative of ongoing star formation activity. The galaxy's overall color suggests a significant population of older stars, with pockets of younger, bluer stars concentrated within the spiral arms. The elliptical shape of the visible galaxy suggests that it is not seen face-on, but at an angle. There is no evidence of any major mergers, but there appears to be some minor disturbance of the disk, giving the spiral arms slightly irregular structure.
