The galaxy appears to be a relatively smooth, elliptical system, exhibiting a somewhat rounded morphology. It presents a concentrated central bulge that seems to dominate the overall light profile. The galaxy displays a yellowish-orange hue, indicative of an older stellar population with minimal ongoing star formation. There is a subtle hint of a possible disk-like structure, although it is not prominently defined. No significant tidal features or indications of a major merger event are apparent.
