The galaxy appears to be a relatively smooth, elliptical galaxy. Its morphology is dominated by a bright, centrally concentrated bulge exhibiting a yellowish-white hue, indicative of an older stellar population. The galaxy appears relatively round in shape, with a gradual decrease in surface brightness moving outward from the central bulge. There are no prominent spiral arms or distinct dust lanes visible, suggesting a lack of significant ongoing star formation. There is a slight blue tinge to the outer regions of the galaxy, possibly indicating the presence of some younger stars but the galaxy generally appears to be a fairly settled system. There is no obvious evidence of any recent or ongoing merger events or tidal disturbances. The overall impression is of a mature galaxy that is near the red sequence.
