The galaxy presents as a disk galaxy observed nearly edge-on. It exhibits a prominent central bulge that appears smooth and spheroidal, with a yellowish hue indicative of an older stellar population. The galactic disk, extending outwards from the bulge, shows a bluer color, suggesting the presence of younger, hotter stars and ongoing star formation, albeit at a relatively low rate. The disk appears relatively thin and elongated, with a high probability of being edge-on and a rounded bulge. There is no obvious indication of major merging activity or significant disturbances in the galaxy's structure. Minor perturbations or disturbances are present. Overall, the galaxy's morphology suggests a relatively undisturbed, mature spiral or lenticular system. The galaxy is estimated to be 3.7 kiloparsecs in radius.
