The galaxy presents a largely smooth, elliptical morphology. The light distribution appears centrally concentrated, with a gradual decrease in intensity outward. The galaxy exhibits a generally rounded shape, deviating only slightly from perfect circularity. There is no clear evidence of spiral arms or a prominent disk structure. The galaxy appears to be in a relatively isolated state, with no obvious signs of ongoing major mergers or tidal disturbances. The galaxy's color profile suggests a stellar population that is dominated by older, redder stars, though there may be some smaller regions of bluer light indicating younger stars or active star formation within the galaxy.
