The galaxy presents as a largely smooth, elliptical object with a concentrated central bulge. The overall shape is highly rounded, exhibiting a nearly circular morphology. There is a lack of any discernible spiral arm structure or prominent dust lanes. Faint extensions of the galaxy's halo are visible at the periphery of the object, gradually fading into the background sky. There is a hint of a disk, with the colours appearing slightly bluer towards the outskirts than in the centre. The galaxy shows no obvious signs of ongoing major merger activity or tidal disruption. Its estimated size suggests it is an average galaxy and its luminosity indicates it is a reasonably bright galaxy. The colour indices suggest the stellar population is old, with a relatively low star formation rate. The lack of morphological disturbances suggests a relatively undisturbed evolutionary history.
