The galaxy presents as a relatively smooth, elliptical structure. The core is a bright, concentrated yellow-white, indicating an older stellar population likely dominated by evolved stars. Moving outward from the core, the color gradually transitions to a reddish hue, possibly indicating a diminishing presence of younger, bluer stars. The galaxy appears to have some mild disturbances in its outer regions, as some parts of the edge of the visible disk are not smooth. The observed color suggests a low rate of ongoing star formation. The galaxy does not display a pronounced disk or spiral arm structure. It exhibits a generally elliptical morphology. The overall appearance suggests a significant mass and an evolved state, likely undergoing little to no major merging events.
