The galaxy presents a largely smooth, elliptical morphology, displaying a concentrated central bulge that is more luminous than its surrounding regions. A subtle color gradient is observed, with the core exhibiting a yellowish-white hue, potentially indicative of an older stellar population. There is a very slight elongation in its shape, appearing to be somewhere between round and cigar shaped. No distinct spiral arms or prominent dust lanes are observed. The overall structure suggests the galaxy is relatively undisturbed.
