The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears largely spheroidal, lacking significant disk-like features or spiral arm structures. The light distribution suggests a high degree of radial symmetry, with no obvious elongation or asymmetry. The color profile appears somewhat uniform across the galaxy, trending towards the redder end of the spectrum, indicating a likely older stellar population. There is no evidence of recent major merger events or significant tidal disturbances. The galaxy's apparent size is relatively compact, suggesting a physically smaller object or significant distance. The overall appearance points towards classification as an elliptical galaxy.
