This galaxy presents a largely smooth, elliptical morphology. Its core exhibits a concentrated, bright yellow-white hue, indicative of an older stellar population. The isophotes appear generally round, displaying minimal ellipticity. Fainter, diffuse extensions emanate from the central region, fading into the background sky. No prominent spiral arms or distinct features are discernible, suggesting a lack of significant ongoing star formation. There is no evidence of tidal tails or morphological disturbances to suggest recent or ongoing merger events. The overall color gradient suggests a red-sequence galaxy, consistent with a population of older, less massive stars. 
