The galaxy presents a largely smooth morphology. The central region exhibits a high concentration of light, appearing almost uniformly bright with a yellowish hue, suggesting an older stellar population. Moving outwards, the light distribution decreases gradually without any distinct spiral arm features or prominent dust lanes visible. There's a subtle color gradient, with the outer regions showing a slightly bluer tint compared to the core, possibly indicating the presence of some younger stars, but at a low rate. The overall shape appears close to circular, with no obvious signs of significant tidal distortions or ongoing mergers. There is a slight hint of a flattened disk. The galaxy seems to be an elliptical, but more data would be needed to completely rule out a spiral.
