The galaxy presents as a relatively smooth, elliptical structure with a centrally concentrated bulge. A subtle color gradient is apparent, transitioning from a yellowish-white core to a bluer outer region. No distinct spiral arms or dust lanes are readily visible. The galaxy exhibits a nearly circular morphology, with minimal elongation or distortion. There is no indication of significant tidal disturbances or ongoing mergers. Overall, the galaxy appears to be a mature system with a dominant spheroidal component, likely indicative of a high stellar mass and relatively low specific star formation rate.
