The galaxy presents as a relatively face-on spiral system with a distinct, although somewhat ill-defined, disk structure. There's a noticeable central bulge, slightly elongated and brighter compared to the outer disk regions. The spiral arms are not sharply defined but are suggested by subtle color and brightness variations within the disk. Overall, the galaxy exhibits a bluish hue, indicative of ongoing star formation, although the specific star formation rate appears to be low to moderate. The disk seems relatively smooth, hinting at a potentially flocculent spiral arm structure rather than grand design spiral arms. There are no obvious signs of a major merger or significant tidal disturbance. However, some subtle asymmetries within the disk might suggest minor interactions or internal dynamic processes. The morphology leans towards a spiral galaxy, with characteristics of a possibly late-type spiral showing only minor disturbance.
