The galaxy presents a clear spiral structure, with tightly wound arms emanating from a central bulge. The bulge exhibits a yellowish-red hue, suggesting an older stellar population. The spiral arms show a bluer tint, indicative of ongoing star formation. The galaxy has a moderate inclination relative to our line of sight. There are some indications of minor disturbances, but the galaxy overall presents a relatively well-defined spiral morphology. The central bulge appears small in comparison to the disk.
