The galaxy presents as an elongated, disk-like structure, viewed nearly edge-on. The central bulge appears relatively bright and concentrated, exhibiting a yellowish-white hue, suggestive of an older stellar population. Extending outwards from the bulge, the disk component displays a bluer color, indicative of ongoing star formation. The disk shows some irregularities, but no obvious signs of strong tidal interactions or major disturbances. Overall, it appears as a relatively undisturbed spiral or lenticular galaxy.
