The galaxy presents an elliptical morphology, elongated along its major axis. It exhibits a smooth, featureless appearance with no distinct spiral arms or bar structure visible. The light distribution appears centrally concentrated, indicating a prominent bulge component. The galaxy's color profile suggests a population of older stars, as evidenced by the reddish-orange hue in the central regions. The outer regions show a bluer tint, potentially indicative of some ongoing, albeit low-level, star formation. There is no apparent evidence of tidal disturbances or ongoing mergers, suggesting a relatively undisturbed evolutionary history. The overall structure suggests a relatively evolved galaxy, transitioning towards a quiescent state.
