The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, appearing brightest at its core and gradually fading towards the edges. The color is predominantly yellowish-orange, suggesting an older stellar population with relatively low ongoing star formation. There is a subtle elongation present. No distinct spiral arms or bar structures are discernible. There is a suggestion of minor asymmetry in the outer regions, hinting at a potential past interaction or minor disturbance, although the resolution limits detailed analysis. The galaxy appears to be relatively isolated.
