The galaxy presents as a relatively smooth, elongated structure, likely an elliptical or lenticular galaxy viewed at an angle. There is a concentration of light in the central region, suggesting a bulge. The light appears to fade gradually outwards, with no evidence of spiral arms or prominent dust lanes. The overall color is indicative of an older stellar population. There is some evidence of minor disturbances in the outer regions. The galaxy does not appear to be undergoing a major merger event.
