The galaxy presents as a relatively small, elliptical object. The light distribution appears smooth and centrally concentrated, with a subtle elongation along one axis, giving it a somewhat lenticular or "in-between" shape. There is a marginal indication of bluer light emission concentrated toward the center, potentially suggestive of recent or ongoing star formation, although its contribution to the overall luminosity seems minor. No prominent spiral arms or distinct disk-like structure are discernible. The galaxy lacks any obvious signs of tidal disturbances or ongoing merger activity, based on visual inspection. Overall, the morphology is consistent with a galaxy dominated by an older stellar population, but with the possibility of some residual star formation in the central region.
