The galaxy presents an elliptical morphology, elongated along a major axis oriented approximately north-south. A central bulge is evident, appearing bright and concentrated with a yellowish hue, suggesting an older stellar population. The disk component exhibits a bluer color, indicative of younger stars and ongoing star formation, though this activity is less prominent than that of other galaxies. The outer regions of the galaxy gradually fade into the background sky, showing a diffuse halo structure. There is some indication of a subtle tidal stream or faint shell-like structure along the major axis of the galaxy, suggesting a previous minor merger event or interaction, although the galaxy predominantly appears undisturbed. Overall, the galaxy seems to be an elliptical galaxy that is possibly undergoing morphological evolution due to a past event.
