The galaxy presents as a moderately bright, relatively small object. Its morphology appears predominantly smooth, with some subtle features suggesting a disk-like structure. The overall shape leans towards round, although not perfectly spherical; there's a slight elongation. There's no strong indication of a major ongoing merger, but subtle disturbances imply possible minor interactions or internal dynamics. Color analysis indicates higher presence of red light. This suggests an older stellar population with a relatively low star formation rate. Considering its size, luminosity, and overall characteristics, this galaxy is likely an elliptical, potentially with a weak disk component.
