The galaxy presents as a spiral galaxy, inclined somewhat to our line of sight. Evidence of spiral arm structure is visible, albeit somewhat diffuse. The arms appear somewhat patchy, suggestive of regions of active star formation. The central bulge is prominent, displaying a moderate size relative to the overall galactic disk. The bulge exhibits a smooth, yellow hue, which may indicate an older stellar population. The disk shows a bluer coloration, especially towards the edges, which aligns with expectations for ongoing star formation. There are no prominent distortions or tidal features that would suggest a major recent merger event. The disk appears somewhat asymmetric, which could be due to minor gravitational interactions. Overall, the galaxy presents as a fairly typical spiral galaxy experiencing moderate levels of star formation.
