The galaxy appears as a disk galaxy, viewed nearly edge-on. There is a noticeable central bulge, which seems quite prominent. The disk shows a yellow hue, which indicates an older stellar population. There is a slight asymmetry in the disk's light distribution, potentially suggesting minor interactions or internal disturbances. There is a possible merging event, with a disturbance occurring. The overall morphology implies a relatively massive system with a subdued star formation rate.