The galaxy presents as a centrally concentrated, elliptical morphology. The light distribution is smooth and exhibits a radial gradient, with the core appearing brighter and more intensely colored in reddish hues, suggesting an older stellar population dominates the galactic center. There is a gradual decrease in brightness towards the outer edges of the galaxy. Fainter bluish hues appear in the surrounding halo. The overall shape is generally round with hints of ellipticity. There are no apparent signs of spiral arms, bars, or significant dust lanes. The galaxy appears relatively isolated, without any obvious signs of ongoing major mergers or tidal disturbances.
