The galaxy presents as a centrally concentrated, smooth object with an elliptical morphology. A discernible radial color gradient is present, shifting from a relatively redder core to bluer outer regions. There is no obvious spiral arm structure or dust lane obscuration. Faint, diffuse light extends from the central region, gradually diminishing in intensity towards the galaxy's periphery. There are no indications of strong tidal disturbances or a recent major merger event. The galaxy appears relatively undisturbed, with no clear evidence of active star formation based on the light present. The light is consistent with an older stellar population that is not forming many young blue stars.