The galaxy presents as a fairly smooth, elliptical-like structure. It is observed as a concentrated central bulge with a diffuse halo extending outwards. The color profile appears to be largely homogenous, with a slight gradient towards redder hues in the central region, suggesting an older stellar population. There is no obvious spiral arm structure or prominent dust lanes visible. The galaxy displays a high degree of roundness in its morphology. There is no evidence of major mergers or significant tidal disturbances in the immediate vicinity. The overall form suggests a system that has largely completed its major evolutionary processes.
