The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a pronounced, bright core, likely indicative of a high concentration of stars and possibly a supermassive black hole. The light distribution fades gradually from the center outwards. There may be some subtle perturbations in the outer regions, perhaps related to minor gravitational interactions or internal dynamics. The galaxy exhibits a reddish-yellow hue, suggesting an older stellar population with a lower rate of ongoing star formation. The overall morphology does not show clear evidence of spiral arms or a well-defined disk structure.
