The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. The light distribution is centrally concentrated, fading gradually outwards. The color profile appears redder in the central region, suggesting an older stellar population with less ongoing star formation in the core. Fainter, bluer extensions are visible along the major axis, potentially indicating regions of more recent star formation or tidal features. There are minor irregularities in the outer regions of the galaxy, possibly indicating minor gravitational interactions or mergers. The galaxy exhibits a slight elongation, but it is mostly spheroidal in shape.
