The galaxy presents an elliptical morphology, elongated along a defined axis. It exhibits a smooth, centralized concentration of light, indicative of a prominent bulge. The luminosity appears to decline gradually from the core outwards, lacking any distinct spiral arm structures or prominent dust lanes. The overall color appears to be on the redder side, suggesting an older stellar population, with no large amounts of star formation occuring. There is no evidence of any recent merger activity. The galaxy appears relatively undisturbed.
