The galaxy presents as a largely smooth, elliptical-like structure. A concentrated central bulge is apparent. The galaxy exhibits a yellow-orange hue across the visible spectrum, which could indicate a relatively older stellar population within the bulge. The outer regions of the galaxy appear more diffuse, transitioning into the background sky with no readily discernible spiral arm structure. There appears to be minor or no merging or tidal disruption occurring in this galaxy, according to the morphology. The lack of significant blue coloration could suggest a low rate of recent star formation across the galaxy. There appears to be a gradual decrease in luminosity from the center outwards, which could indicate the density of stars in the bulge area. The general smoothness of the object and absence of any notable features suggest a stable and relatively evolved galaxy structure.
