The galaxy presents a somewhat elliptical morphology, with a noticeable bulge component. The bulge exhibits a yellowish-white hue, suggestive of an older stellar population. The galactic disk appears less defined, with a smoother, less structured appearance compared to typical spiral galaxies. There is an indication of some bluer regions in the disk, indicating the presence of younger, hotter stars, but they are not prominent. The overall color profile suggests that this galaxy is an intermediate type, somewhere between a spiral and an elliptical galaxy. There seems to be some dust absorption around the center of the bulge, though faint, and no sign of interactions or major disturbances. The galaxy is significantly tilted relative to our line of sight.
