The galaxy presents as a moderately inclined disk galaxy, with an elliptical shape. It exhibits a bright, concentrated central bulge, appearing smooth and yellowish-white in color. The disk component displays a more diffuse and somewhat mottled appearance, with a bluer hue than the central bulge, suggesting the presence of younger stellar populations. There may be a faint dust lane or some obscuring material present in the disk, especially in the area adjacent to the brighter bulge. There is no evidence of strong spiral arm structure or intense star formation regions, instead, the disk appears relatively featureless and homogenous. The overall morphology hints at a galaxy undergoing a process of fading or quiescence, transitioning from a more actively star-forming state to a more passively evolving state. The red shift implies this galaxy is reasonably close, and therefore a good target for future study.
