The galaxy presents a centrally concentrated, elliptical morphology. It exhibits a smooth, diffuse light profile, suggesting an evolved stellar population. The color appears to be primarily yellow-red, indicating a lack of significant ongoing star formation and a dominant population of older, redder stars. There is a slight asymmetry or minor disturbance in the outer regions. The galaxy appears to be relatively isolated, with no signs of major mergers or strong tidal interactions. Overall, it appears to be a passively evolving, massive galaxy.
