The galaxy presents a predominantly smooth, elliptical morphology. Its light profile exhibits a concentrated, centrally bright core that gradually fades outwards. The core appears yellowish, suggestive of an older stellar population. There is little to no evidence of spiral arms or active star formation regions. No distinct dust lanes are apparent. The overall shape is largely round, though with a slight elongation along one axis. There may be a slight disturbance present, with a hint of asymmetry in the outer regions, possibly indicating a minor interaction or recent merger. The color gradient suggests that the galaxy is relatively quiescent, with only low levels of current star formation.
