The galaxy appears to be a spiral galaxy, viewed at a steep inclination. The central bulge is prominent and has a smooth, concentrated appearance, exhibiting a yellow-orange hue. Traces of spiral arm structure are visible extending from the bulge, appearing somewhat disrupted or diffuse. The outer regions of the galaxy show a bluer tint, possibly indicating regions of younger stellar populations. Overall, the galaxy presents an elliptical profile, with an axial ratio indicating a flattened shape when viewed face-on. There is no obvious evidence of a major ongoing merger, although some minor morphological disturbances cannot be ruled out.
