The galaxy presents as a mostly smooth, elliptical-like structure with a concentrated central bulge. Its shape is elongated, appearing somewhere between round and cigar-shaped. The light distribution suggests a relatively old stellar population, particularly in the central regions. The color profile seems to be redder in the core, with a gradual shift towards slightly bluer hues in the outer regions, possibly indicating some degree of ongoing or recent star formation in the galactic disk, though at a low rate. There is no obvious evidence of major mergers or significant tidal disturbances in this image.
