The galaxy appears to be a spiral galaxy, presenting a nearly face-on orientation. It exhibits a bright, concentrated central bulge that transitions to a diffuse disk. The spiral arms are not sharply defined, showing a somewhat flocculent structure. There is evidence of ongoing star formation, as indicated by the faint blue hues within the spiral arms and the diffuse disk. The overall color suggests a relatively mature stellar population, with a dominant yellow/orange hue in the central regions indicative of older stars, with a hint of younger, bluer stars tracing the spiral arms. There seems to be minor disturbances in the structure, but overall, it is a relatively undisturbed and isolated spiral galaxy.
