The galaxy presents as a smooth, elliptical morphology, with a relatively high degree of symmetry. The light profile appears centrally concentrated, showing a gradual decrease in intensity moving outward from the core. The core exhibits a pronounced yellowish hue, suggesting a population of older stars. The outer regions display a slight bluer color, hinting at more recent star formation, although this activity is not overtly prominent. There are no visually apparent spiral arms or strong indications of active starburst regions. There does not seem to be any major merging going on, but it is possible there is a small minor disturbance. The object has an intermediate roundness.
