The galaxy appears to be a spiral galaxy, viewed at an angle between edge-on and face-on. The central bulge is prominent and exhibits a yellowish hue, potentially indicating an older stellar population. There is a visible disk component with hints of spiral arm structure. One arm appears more prominent than the others. The arm also appears to have a bluer color, indicative of younger stars. A portion of the disk appears slightly disturbed or warped. The galaxy shows some signs of past or ongoing minor interactions.