The galaxy presents as a centrally concentrated, smooth object with a discernible, though not sharply defined, edge. The overall shape appears largely elliptical, exhibiting a high degree of circularity. The color profile is generally consistent across the galaxy, with a subtle shift towards redder hues in the central regions. There is no immediately apparent spiral structure or the presence of dust lanes. The overall impression is that of a relatively undisturbed system. There is no strong evidence of ongoing major merger activity, although subtle irregularities could be indicative of minor interactions.
