The galaxy presents as a relatively smooth, elliptical-like structure. It has a concentrated central bulge, with a gradual decrease in luminosity towards the outer edges. The color appears generally yellowish-orange, indicative of an older stellar population with a dearth of active star formation. There is no clear evidence of spiral arms or a defined disk. A slight elongation is observed, deviating from a perfectly circular shape. Some faint disturbances are visible in the outer regions, which could be indicative of a past minor merger event. The galaxy's overall morphology suggests it is a massive, evolved system.
