The galaxy presents a smooth, elliptical morphology. Its shape is somewhat elongated, appearing more cigar-shaped than perfectly round. The central region exhibits a high concentration of light, with colors suggesting an older stellar population. Fainter, more diffuse light extends outwards from the core, diminishing gradually with radial distance. There are subtle hints of asymmetry in the outer regions, but no strong evidence of spiral arm structure or major disturbances indicative of ongoing mergers. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
