The galaxy presents as a disk galaxy, likely a spiral, oriented somewhat edge-on relative to our line of sight. A prominent bulge region dominates the central part of the galaxy, appearing to be of moderate size. This central bulge exhibits a yellow-white color, suggesting an older stellar population. The disk component of the galaxy is more diffuse, with hints of spiral arm structure visible. There is a strong suggestion of a central bar feature bisecting the bulge. The outer regions of the disk show a bluer tint, potentially indicating regions of active star formation. No major mergers or disturbances are immediately apparent in the galaxy's morphology, although minor disturbances cannot be ruled out. 
