The galaxy appears as a relatively smooth, elliptical structure with a bright central bulge. The light distribution suggests a high degree of radial symmetry. The galaxy is elongated, exhibiting a cigar-like shape, with a lack of any strong spiral arm features or prominent dust lanes. There are hints of some color variation, with the central region appearing slightly yellower compared to the bluer outer regions. There is no indication of any significant ongoing merger activity or major morphological disturbances. The overall appearance suggests a relatively evolved system.
