The galaxy appears to be an elliptical galaxy, exhibiting a smooth, centrally concentrated light profile. Its overall shape is largely spheroidal with a slight elongation along one axis. The core region demonstrates a significantly higher luminosity than the outer regions, with a gradual decrease in brightness radiating outward. While the galaxy is primarily smooth in appearance, subtle color variations are present. The central regions exhibit a yellowish-white hue, suggesting an older stellar population. Fainter, more diffuse blueish regions appear to be present in the outer edges, likely indicating regions of more recent, albeit low, star formation. There is no strong evidence of spiral arm structures or significant dust lanes. No signs of ongoing merging activity or major tidal disturbances are immediately apparent.
