The galaxy presents as a generally smooth, centrally concentrated object. Its morphology suggests a likely classification as an elliptical galaxy, though there is some possible faint disc-like structure. There is no noticeable dust lane or arm structure. The galaxy exhibits a color gradient, with a brighter, yellowish-white core gradually fading to a dimmer, redder outer halo. This color gradient potentially indicates an older stellar population in the core and the presence of ongoing or recent star formation in the extended disk region. The object shows no major signs of ongoing merger activity or significant tidal disturbances. The galaxy is somewhat elongated in shape.
