The galaxy exhibits a predominantly smooth morphology, with a high degree of central concentration. The shape appears nearly round, with a minor deviation toward a slightly elliptical form. There is some indication of internal structure, possibly suggestive of minor disturbances or tidal features, though the dominant impression is of a largely undisturbed system. Color gradients are present, with a redder core potentially indicating an older stellar population or significant dust obscuration. Some blue light is present in less concentrated spots, possibly from a small number of more active star forming regions. There are no signs of a major merger, although a minor interaction cannot be ruled out. The galaxy presents as a relatively massive system.
