The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central region, surrounded by a more diffuse halo. The galaxy is nearly circular in appearance, displaying minimal evidence of a disk structure or significant tidal disturbances. There is a notable lack of prominent features such as spiral arms or dust lanes. Color gradients suggest a possible redder core compared to its outer regions, indicative of an older stellar population residing within the galactic nucleus. Faint surrounding light suggests the presence of an extended stellar halo. There appears to be minimal ongoing star formation activity; the overall color profile suggests a largely quiescent galaxy. 
