The galaxy presents as an elliptical morphology, exhibiting a relatively smooth and featureless appearance. The central region displays a concentration of light, indicative of a prominent galactic nucleus. There is a noticeable radial decrease in luminosity from the core to the outer regions. The overall color profile is suggestive of a more evolved stellar population, trending towards the redder end of the spectrum. There's no visible evidence of spiral arms or a distinct disk structure. The shape appears approximately round, with only minimal deviation from perfect circularity. There are no obvious signs of ongoing major merger activity or significant tidal disturbances.
