This galaxy exhibits a clear disk structure with discernible spiral arm features. The central bulge appears moderately sized, contributing a significant amount of light to the galaxy's overall luminosity. The spiral arms appear somewhat tightly wound, originating from the central bulge. The bluer colors observed in the disk suggest ongoing star formation activity, primarily located within the spiral arms. The galaxy does not appear to be undergoing a major merger event, although some minor disturbances cannot be ruled out. There may be a weak bar structure present, but its presence isn't definitive. The overall morphology aligns with that of a late-type spiral galaxy. The galaxy is relatively close.
