The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, displaying a somewhat elongated structure without any apparent strong bar or spiral arm features. The color is predominantly blue-white, suggesting a population of relatively young, hot stars and ongoing star formation activity. No obvious dust lanes or distinct features associated with recent major merger events are discernible. There is a hint of minor disturbance present in the galactic disk, which might indicate a minor merging event.
