The galaxy presents as a single, largely homogenous object, with an elliptical morphology that suggests a spheroid-dominated structure. The light distribution appears smooth and centrally concentrated. It possesses a diffuse, but clearly defined, central bulge and a halo that gradually fades into the background sky. The galaxy exhibits a yellowish-white color, potentially indicating a population of older stars with minimal recent star formation. There might be slight irregularities or minor disturbances in its morphology, potentially hinting at past or ongoing interactions or merger events.
