The galaxy presents a generally smooth morphology, appearing largely spheroidal in shape. It exhibits a bright central bulge that dominates the overall luminosity. The light distribution gradually decreases from the core outwards, with no discernible spiral arms or strong features such as bars or rings. There's some indication of minor disturbances with a small feature possibly interacting to the right of the galaxy. The colors indicate relatively low levels of star formation, with a population of aging stars contributing to the redder hues, although a bluish tint toward the center suggests the presence of a younger population of stars. Overall, the galaxy appears as a relatively evolved system.
