The galaxy presents an elliptical morphology with a relatively smooth light distribution. The central bulge is bright and concentrated. There's an indication of a faint, extended disk or halo surrounding the bulge. The light distribution fades significantly with increasing radius. The colors suggest an older stellar population. The galaxy exhibits a slight elongation, but is generally round in appearance. A smaller, possibly interacting, object is visible nearby. There is no discernible evidence of prominent spiral arms or significant dust lanes.
