The galaxy presents as a roughly elliptical structure with a bright, concentrated central bulge. The bulge exhibits a smooth, yellowish-white color, suggesting an older stellar population. The outer regions of the galaxy display a fainter, bluer hue, potentially indicating the presence of more recent star formation. While appearing generally smooth, there is a subtle suggestion of a disk-like structure oriented at a slight angle to our line of sight. The overall morphology appears relatively undisturbed, lacking any obvious signs of a major merger event, though minor tidal disturbances cannot be ruled out. The galaxy's redshift suggests it is at a considerable distance, yet its apparent magnitude indicates it is intrinsically luminous.
