The galaxy presents as a relatively smooth and concentrated object. Its overall morphology appears elliptical or lenticular. The light distribution suggests a dominant bulge component, exhibiting a radial intensity profile that peaks centrally. There is no evidence of prominent spiral arms or a distinct disk structure, but there is a very slight elongation in its shape. Color gradients across the galaxy appear subtle. The central region appears bluer, potentially indicating a small amount of recent or ongoing star formation, although the overall color suggests a more evolved stellar population. No strong signs of tidal disturbances or ongoing merger activity are visible.
