The galaxy presents a distinct spiral structure. Traces of spiral arms are observable, though somewhat diffuse and patchy, originating from a moderately sized central bulge. The bulge appears yellowish in color. The arms are somewhat flocculent, with blue hues indicating the presence of ongoing star formation. The galaxy disk is not viewed edge-on, but rather at an angle, allowing clear visualization of the arm structure. No prominent bar structure is discernible at its center. There are some irregular features within the disk, hinting at possible minor disturbances but no clear evidence of an advanced merger stage.
