The galaxy presents as a lenticular or early-type spiral with a prominent central bulge that dominates its overall luminosity. The bulge exhibits a smooth, relatively featureless appearance. Surrounding the bulge, a flattened disk is observed. This disk is not highly resolved, but there are subtle indications of spiral structure present, perhaps tightly wound arms. Some slight disturbances may be evident in the disk, indicating minor interactions or internal processes. The galaxy is not viewed edge-on, as the disk is presented somewhat face-on but at an angle, allowing for an estimation of the galaxy's inclination. Light from the galaxy is strongest in the redder parts of the spectrum, possibly caused by older stellar populations. Overall, it presents as a galaxy undergoing a transitional stage between a spiral and an elliptical galaxy.
