The galaxy presents as a relatively smooth, centrally concentrated object. The overall morphology appears elliptical, with a high degree of roundness observed. There is a notable color gradient, with the central region exhibiting a yellowish hue, transitioning to a slightly greenish tinge in the outer regions of the galaxy. No distinct spiral arm structures or bar features are discernible. There is no obvious evidence of tidal streams or ongoing mergers. The galaxy appears relatively isolated and undisturbed. The light profile suggests an older stellar population with some ongoing star formation.
