The galaxy presents as a disk-shaped system, viewed nearly edge-on. A prominent central bulge is apparent, exhibiting a yellowish hue, possibly indicating an older stellar population. The disk appears slightly warped or distorted, possibly due to interactions. The disk itself displays a mottled texture, suggesting areas of active star formation interspersed with regions of lower stellar density. A blueish tint pervades the outer regions of the disk, which could indicate the presence of younger, hotter stars. The overall structure exhibits a moderate degree of disturbance, with no clear signs of a major ongoing merger event.
