The galaxy presents a predominantly smooth, elliptical morphology. The color profile indicates an older stellar population, with a yellowish-orange hue concentrated towards the galactic center. The central bulge appears bright and relatively compact, gradually fading into the outer regions. There's a slight hint of bluer tones in the outer regions, suggesting the presence of some younger stars. No distinct spiral arms or prominent dust lanes are visible, further supporting its classification as an elliptical galaxy. The galaxy appears relatively isolated, showing no obvious signs of recent or ongoing major mergers or tidal disturbances.
