The galaxy presents as a centrally concentrated, smooth object with a generally elliptical morphology. The light distribution indicates a dominant, spheroidal component. There is a slight elongation but it appears mostly round. Color gradients are subtle, with a suggestion of bluer hues at the faint edges and a more yellowish-white core, possibly indicative of an older stellar population dominating the central region. No distinct spiral arm structures or dust lanes are discernible. The galaxy exhibits minimal signs of recent or ongoing merger activity, no tidal tails or significant disturbances are apparent in its overall structure. Based on these characteristics it can be inferred to be an elliptical or lenticular galaxy at a moderate redshift.
