The galaxy presents as an elliptical morphology, appearing largely smooth and well-resolved. The central region exhibits a high degree of luminosity, indicating a dense concentration of stars. The light gradually fades towards the outer edges, with no apparent spiral arms or distinct features. The overall color profile suggests a population of older stars, emitting light primarily in the redder wavelengths. There is a minimal indication of ongoing star formation. The galaxy appears relatively undisturbed, showing no signs of major merger events or significant tidal disruptions. It exhibits a generally rounded shape.
