The galaxy presents a prominent disk-like morphology, exhibiting evidence of spiral arm structure. The arms appear somewhat flocculent, rather than grand design, with varying degrees of definition. There's an indication of a central bulge, not overly dominant. The overall color profile suggests a mix of stellar populations. There is likely ongoing or recent star formation in the disk, as evidenced by regions of bluer color, while the bulge appears more yellow/white, indicative of an older stellar population. There isn't a strong indication of a central bar structure. No signs of significant tidal disturbance or ongoing major merger activity are readily apparent. The disk appears relatively undisturbed.