The galaxy presents a largely smooth and elliptical morphology. Its overall color appears to be reddish-orange, indicative of an older stellar population. The galaxy's light profile exhibits a centrally concentrated bulge that fades gradually into the outer regions. There is no clear evidence of spiral arm structures or distinct features indicative of ongoing active star formation. The galaxy is relatively compact and lacks any signs of major tidal disturbances or ongoing mergers. A slight asymmetry may be present, warranting further investigation.
