The galaxy appears as a somewhat elongated, lenticular or early-type spiral galaxy, with a relatively smooth light distribution. A concentrated central bulge is visible, fading gradually outwards towards the edges. The overall color is skewed towards the redder part of the spectrum, indicating an older stellar population within the galaxy, with little recent star formation. There might be a faint disk component, but it is not clearly resolved. The morphological characteristics seem to show this is a system that is stable and not undergoing a major merger. Some minor distortions are likely present.
