The galaxy presents as a relatively smooth, elliptical morphology. Its light profile appears concentrated towards the center, indicating a significant bulge component. The central region is notably bright and yellowish-orange in color, suggesting an older stellar population. There is a subtle extension or asymmetry in the light distribution on one side, hinting at possible tidal interactions or recent minor mergers. Overall, the galaxy appears largely undisturbed, exhibiting a regular and well-defined structure. The estimated physical size suggests a fairly massive galaxy. Based on color and morphology, star formation activity appears relatively low.
