The galaxy presents a generally smooth and elliptical morphology. The central region is noticeably brighter and exhibits a yellowish hue, which could indicate an older stellar population. There is little to no evidence of prominent spiral arms or a distinct disk structure. The overall shape appears relatively circular, with no signs of major mergers or significant tidal disturbances. Faint, diffuse light extends outward from the core, suggesting a gradual decline in stellar density with increasing radius. The lack of blue hues implies a suppressed rate of active star formation within the galaxy.