The galaxy presents as an elongated, disk-shaped structure, likely viewed at a high inclination. The central bulge appears yellowish-orange, indicating an older stellar population. Moving outward from the center, the disk shows a transition to bluer hues, suggesting the presence of younger, hotter stars and regions of active star formation within the spiral arms, although these arms are not clearly resolved. The galaxy's overall form appears relatively undisturbed, showing no signs of major mergers or significant tidal interactions. The disk extends further along its major axis, gradually fading into the background sky.
