The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. It appears largely featureless, exhibiting a gradual decrease in luminosity from the core outwards. The galaxy's color suggests an older stellar population. There's a very slight elongation, indicating it is not perfectly spherical, but rather somewhat cigar-shaped. There is no indication of any spiral arms or any current merger activity. The light distribution is fairly even, with no strong knots or regions of active star formation immediately apparent. The lack of distinct features suggests it is a relatively evolved system.
