The galaxy exhibits a disk morphology, viewed at an angle that suggests a near face-on orientation. Spiral arm structures are discernible, with what appears to be a two-armed spiral pattern dominating the morphology. The winding of these spiral arms is moderately defined. A prominent central bulge is evident, exhibiting a yellow hue indicative of an older stellar population. The spiral arms appear bluer, suggesting ongoing star formation. There are regions of disturbance, indicating a possibility of interaction or a past minor merger. The overall color suggests a relatively intermediate age stellar population with ongoing star formation in the spiral arms. There's the possible existence of a bar structure, but the prominence is difficult to verify.