The galaxy presents as a somewhat smooth, elliptical-like structure with a notable central bulge. There is evidence of a disk component, although it appears relatively faint and less defined than the central bulge. The galaxy exhibits a slight elongation, with a cigar-like shape. The overall color profile suggests a predominantly older stellar population, indicated by the reddish-yellow hue, especially prominent in the bulge. There is little evidence of active star formation regions from the lack of blue color. No signs of major mergers or significant tidal disturbances are apparent in this image. It appears to be a relatively isolated system without nearby interacting galaxies, although subtle minor disturbances cannot be ruled out.
