The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated bulge, characterized by a yellowish hue, suggesting an older stellar population. Moving outward from the core, the color shifts towards a more greenish-blue, possibly indicating some presence of younger stars or ongoing star formation. The galaxy has a fairly regular, rounded morphology, showing no signs of strong tidal disturbances or major mergers, although a slight asymmetry might indicate minor gravitational interactions. The outer regions of the galaxy fade gradually into the background sky, suggesting a large but diffuse halo component. There is a notable lack of distinct spiral arm structures, supporting its classification as an elliptical galaxy.
