The galaxy presents as a somewhat flattened, elongated structure. Its color is predominantly a warm yellow/orange hue, suggesting a population of older stars. There is a concentration of light towards the center, indicative of a bulge. Faint features or irregularities are potentially observed along the major axis, and there is a faint, diffuse component extending away from the central region, but it is somewhat disturbed. It does not appear to be undergoing a major merger, although there appears to be some kind of interaction occurring.
