The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge and lacks any prominent spiral arm structure or distinct features indicative of active star formation. The core region displays a yellowish-orange hue, potentially indicating an older stellar population dominated by redder giants and supergiants. The galaxy's color becomes progressively bluer towards its outer regions, suggesting the presence of a younger stellar population. There is no evidence of an ongoing major merger or significant tidal disturbances. Overall, the galaxy appears to be a relatively undisturbed elliptical system, exhibiting a smooth and largely featureless morphology.
