This galaxy appears to be a spiral galaxy, viewed nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish hue, indicative of an older stellar population. The disk is elongated and relatively thin, showing a somewhat smoother profile. There are suggestions of spiral arm structure, though they are tightly wound and difficult to discern clearly. Based on the appearance, the galaxy doesn't appear to be undergoing any major merger events, although there may be a very slight disturbance in the disk, possibly due to a minor interaction. The disk appears relatively quiescent with minimal star formation currently visible.
