The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal. The light distribution is concentrated towards the center, with a gradual decrease in intensity outwards. The core is bright with a yellow hue, suggesting an older stellar population. The galaxy exhibits no apparent spiral arm structure or prominent dust lanes. There are no signs of ongoing major mergers or significant tidal disturbances, although minor irregularities cannot be ruled out at this resolution. The overall color suggests a lack of significant recent star formation. The galaxy is relatively compact. 
