The galaxy presents as a slightly elongated, disk-shaped structure. The central bulge exhibits a yellow-orange hue, suggestive of an older stellar population with lower ongoing star formation. Moving outwards from the bulge, the disk appears subtly bluer, hinting at the presence of younger, hotter stars within the spiral arms. There may be hints of minor disturbances and perhaps a slight asymmetry in the disk structure. There is an object nearby which may suggest a recent interaction or the presence of a companion galaxy. Overall, it appears as a relatively undisturbed galaxy.
