The galaxy presents a generally elliptical morphology, appearing largely smooth and spheroid in shape. A subtle color gradient is observed, with the central region exhibiting a brighter, yellowish hue, possibly indicative of an older stellar population. The outer regions show a fainter, slightly bluer tint, hinting at the presence of some younger stars or ongoing, albeit subdued, star formation. No distinct spiral arm structures or prominent dust lanes are readily discernible. The overall appearance suggests a relatively evolved system, though not entirely devoid of recent stellar activity. There are some indications that it is undergoing a minor disturbance.