The galaxy presents as an elliptical or lenticular type, displaying a smooth, featureless morphology. It exhibits a prominent central bulge that is approximately 3 kpc across. The light distribution indicates a high degree of central concentration. The outer regions appear fainter, with a gradual decrease in luminosity towards the edges. The color profile is predominantly yellow to white in the core, suggesting an older stellar population. A faint bluish tint is observed within the bulge, hinting at the presence of some younger, hotter stars, perhaps indicating a low level of ongoing star formation. The galaxy has a generally rounded shape, and there are no visible signs of tidal disturbances or mergers with other galaxies.
