This galaxy presents as an elliptical or lenticular structure, appearing elongated with a smooth, diffuse light distribution that diminishes gradually towards the outer edges. The core region exhibits a strong, concentrated luminosity, indicating a likely high density of older stellar populations. Colors range from a pale yellow at the center to a bluish-white in the outskirts. No spiral arms are visible, and there is no distinct dust lane apparent. Overall, the galaxy appears to be relatively quiescent, indicating potentially low ongoing star formation.
