The galaxy presents a generally smooth and elliptical morphology. The central bulge is prominent and exhibits a reddish-orange hue, indicative of an older stellar population. The galaxy appears to be relatively undisturbed, showing no obvious signs of major mergers or tidal features. A faint disk structure appears to surround the bright central bulge. There is no apparent presence of substantial dust lanes or knots of intense star formation within the disk. The galaxy's color suggests it is in the red sequence, and that it has a generally low rate of star formation.
