The galaxy presents a largely elliptical morphology, appearing somewhat smooth in overall texture. There is a noticeable radial color gradient, transitioning from a bluer, likely actively star-forming inner region to redder, older stellar populations in the outskirts. While a disk is not clearly defined, there is a slight flattening visible along one axis, indicating a deviation from perfect sphericity. No prominent spiral arms or dust lanes are observed. The galaxy shows no strong signs of recent or ongoing major mergers or tidal disturbances, appearing relatively undisturbed. The object is compact, with the light profile concentrated towards the center.
