The galaxy presents as a flattened elliptical or lenticular morphology. A central bulge is prominent, displaying a yellowish-white hue, suggesting an older stellar population with diminished star formation. The outer regions exhibit a smoother texture, with faint reddish-brown tones, that could indicate dust lanes or regions of ongoing, albeit low, star formation. The galaxy appears relatively undisturbed, lacking prominent spiral arms or significant tidal features. The overall structure suggests a relatively evolved system, potentially transitioning towards a more passive evolutionary state.
