The galaxy presents as a relatively smooth, disk-shaped structure with a noticeable central bulge. It displays a moderate degree of ellipticity, appearing somewhat elongated along one axis. There is an indication of some spiral arm structure, but it's not well-defined or tightly wound. The color profile suggests a mix of stellar populations. The central bulge shows a yellowish hue, possibly indicative of older, cooler stars, while the disk exhibits a bluer tint, suggestive of ongoing star formation activity. There may be evidence of minor disturbances.
