The galaxy presents as a smooth, elliptical morphology. It exhibits a concentrated central bulge that dominates the overall luminosity. The galaxy displays a color gradient, appearing more yellow-red in the core and gradually transitioning to a slightly bluer hue in the outer regions. This color variation suggests a distribution of stellar populations, with older, redder stars concentrated in the central regions and a younger, bluer population at the edges. There is a slight asymmetry in the outer regions. No distinct spiral arms or other prominent features such as dust lanes are observed. The light profile appears to be smooth and continuous. Overall, this galaxy appears to be an evolved system.
