The galaxy presents as a centrally concentrated system, appearing largely smooth with a high degree of radial symmetry. The core exhibits a bright, yellowish-white hue indicative of an older stellar population. Moving outward from the core, the color gradually shifts towards a redder and fainter profile, suggesting a decrease in stellar age and/or metallicity in the outer regions. There are hints of slight disturbances in the outer regions of the galaxy, but no clear indications of significant ongoing merger activity or major morphological disruptions are immediately visible. The overall shape is elliptical, with a high degree of roundness, appearing nearly circular on the plane of the sky. Star formation is present, but at a moderate level. The estimated mass range is relatively high, indicative of a large galaxy. 
