The galaxy presents as an elliptical morphology, displaying a smooth, centrally concentrated light distribution. The light profile indicates a spheroid-dominated system with minimal discernible disk-like features or spiral arm structures. There is a slight elongation to its shape. The galaxy's color indices suggest a population dominated by older stars, as the central region exhibits a yellowish hue, indicative of reduced star formation. Hints of bluer colors can be observed in the outer regions which may indicate some ongoing star formation, but at a low rate. No significant tidal features or signs of recent major merger events are readily apparent. The overall impression is of a relatively quiescent, evolved galaxy.
