The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. Its color profile indicates a likely older stellar population, exhibiting a yellowish-orange hue. There is no discernable spiral structure or prominent dust lanes. The overall shape is largely spherical, showing a high degree of roundness with only slight deviations from perfect symmetry. Evidence of recent or ongoing major mergers is not apparent; however, subtle irregularities in the outer regions cannot be entirely ruled out given the image resolution. This galaxy exhibits characteristics consistent with a quiescent or passively evolving system, with a low star formation rate. 
