The galaxy presents as a slightly elliptical, relatively smooth object, with a concentrated central bulge region exhibiting a yellowish-white hue, suggesting a population of older stars. This bulge is surrounded by a fainter disk. The disk shows some evidence of slight asymmetry or disturbance. The overall color suggests a low star formation rate for the galaxy, which is consistent with a more evolved system. There is also a potential tidal feature, such as minor disturbance or possible merger, present in the form of a slight disruption or asymmetry in the galaxy's outer regions. 
