The galaxy appears to be a disk galaxy, oriented nearly edge-on from our line of sight. A prominent bulge is visible at the center, exhibiting a smooth, concentrated light profile with a yellowish-orange hue. There is evidence of a disk component, seen as a faint, elongated structure extending outwards from the central bulge. This structure appears relatively smooth and without obvious spiral arm features in this image. A slight asymmetry or minor disturbance is suggested by the subtle warp in the disk plane. Additionally, there may be some evidence of merging or tidal interaction suggested by the subtle disturbances in the morphology of the faint and diffuse outer regions of the disk.
