The galaxy presents a generally smooth, elliptical morphology with a concentrated central bulge. It exhibits a yellow hue in the core region, suggesting an older stellar population. The galaxy appears relatively round. There is no strong visual evidence of spiral arms or a prominent disk structure. Faint blue tinges around the very exterior of the galaxy suggest the presence of some younger stars or active star formation regions, although these are not pronounced. There is no indication of significant ongoing merger activity or major disturbances in the overall structure. The galaxy appears to be a relatively isolated system, with a fairly uniform and quiescent morphology.
