The galaxy presents as a relatively smooth and rounded structure. It exhibits a concentrated central region with a gradual decrease in luminosity outwards, suggesting a possible elliptical morphology or a lenticular galaxy with a prominent bulge. There's little evidence of spiral arms or significant dust lanes, which supports a classification leaning towards early-type galaxies. The color appears generally redder, which could indicate an older stellar population with fewer young, massive stars and ongoing star formation. There's a subtle hint of a surrounding halo or extended component, though it's faint and not clearly defined. The overall texture of the galaxy appears homogenous.
