The galaxy presents a distinct spiral structure, with arms that appear tightly wound around a central bulge. The bulge exhibits a moderate size relative to the overall galactic disk. There is a suggestion of a bar-like structure crossing the center of the bulge. The spiral arms display a mottled texture, possibly indicating regions of active star formation. The overall color gradient suggests a mature stellar population within the central bulge, with bluer hues dominating the spiral arms, indicative of younger, hotter stars. The galaxy does not appear to be undergoing any major merger events, although there might be minor disturbances in the outer regions of the disk. The disk is not observed edge-on but is face-on.
