The galaxy presents a largely elliptical morphology, exhibiting a smooth, featureless appearance. The core region displays a concentrated intensity, suggestive of an older stellar population. A subtle transition in color is observed from the central region outwards, shifting from a yellowish-red hue at the center to a faint blue surrounding the core. There are no apparent spiral arm structures, bar features, or indications of ongoing major merging events. Minor irregularities are not obviously apparent. The galaxy shows rotational symmetry and is slightly elongated along one axis.
