The galaxy presents as a primarily smooth, centrally concentrated object. It exhibits a largely elliptical morphology, appearing almost perfectly round in projection. There is a noticeable radial color gradient, shifting from a yellowish-white core to a more bluish-tinged outer region. No distinct spiral arm structure or prominent dust lanes are discernible. Faint disturbances might be present suggesting the possibility of a minor recent merger but these are not well defined. The light profile suggests an evolved stellar population, particularly concentrated in the core, possibly a result of minimal present-day star formation activity. The galaxy appears to be a quiescent, massive system.
