The galaxy presents as a centrally concentrated, elliptical structure with a smooth overall appearance. The core region exhibits a yellowish-white hue, suggesting an older stellar population likely dominated by evolved stars. The surrounding halo displays a bluer tint, hinting at the presence of younger stars and some ongoing, albeit limited, star formation activity. The galaxy does not appear to exhibit any prominent spiral arms or distinct features indicative of a disk galaxy. There is a slight asymmetry visible in the outer regions, possibly indicative of a minor gravitational disturbance or interaction with a smaller companion, although no distinct merging signatures are immediately apparent. The galaxy's overall form is somewhat elongated.
