The galaxy presents as a spiral galaxy, viewed nearly edge-on. A prominent dust lane bisects the galaxy along its major axis, obscuring the central bulge. The galactic disk appears elongated, with a subtle color gradient transitioning from bluer hues at the outer edges to redder tones towards the core. The disk's morphology suggests active or recent star formation in the outer regions, based on the presence of bluer light indicating younger, hotter stars, while the central region suggests an older stellar population and/or dust obscuration. There is no distinct evidence of a major merger event, though some minor irregularities in the disk's structure might suggest a possible interaction. The overall structure suggests the galaxy is relatively undisturbed.
