The galaxy presents a largely smooth, elliptical morphology. The light distribution indicates a centrally concentrated spheroid, with a gradual decrease in luminosity moving outwards from the core. Faint, diffuse extensions are possibly present, though not distinctly separated from the primary body of the galaxy. The color profile reveals a subtle gradient, appearing slightly redder at the core transitioning to bluer hues in the outer regions. There is no apparent spiral arm structure, and the overall form is indicative of an evolved system. There are no features to suggest any major interaction or ongoing merger event. There is an imperceptible elongation of the galaxy, not perfectly circular but instead resembling a more oblate spheroidal shape.
