The galaxy presents as a centrally concentrated, elliptical or lenticular structure. The core exhibits a bright, yellowish-white hue, suggestive of an older stellar population. Moving outward from the core, the color gradient transitions to a more reddish-orange tone. The outer regions appear relatively smooth with no distinct spiral arm features or obvious dust lanes. The overall shape approximates an ellipse, with a slight deviation from perfect sphericity, appearing somewhat flattened. There is no clear evidence of ongoing major merger activity. Subtle irregularities in the outer regions might suggest minor gravitational interactions or past merger events, though this could be attributed to noise.
