The galaxy presents as a somewhat elongated, elliptical structure. A concentrated, bright central bulge is apparent, surrounded by a fainter, more diffuse halo. The halo appears relatively smooth, lacking prominent spiral arms or significant dust lanes. There's a slight color gradient, with the central bulge exhibiting a yellowish hue, suggesting an older stellar population, while the outer regions are slightly bluer, indicating the presence of some younger stars. The shape implies that the galaxy is not viewed perfectly face-on, but rather at a considerable angle. There is no obvious evidence of any major ongoing merger activity or significant tidal disturbances.
