The galaxy presents as an elliptical or lenticular type with a smooth, diffuse appearance. It exhibits a bright central bulge, which transitions gradually into a fainter, more extended halo. The galaxy appears to be relatively undisturbed, showing no strong signs of tidal interactions or major mergers. The color gradients suggest a concentration of older stellar populations towards the core, with a redder hue dominating the central region. Fainter, bluer regions may be present in the outer disk, hinting at some ongoing, albeit low, levels of star formation. The overall morphology suggests a system that has largely exhausted its gas reservoir and is undergoing passive evolution. It has an oval shape, in between round and cigar shaped.