The galaxy presents as an elliptical morphology, with a smooth, relatively featureless appearance. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer regions. There is a subtle color gradient noticeable, with the central region exhibiting a slightly yellower hue compared to the outer regions, which appear more blue/green. The overall structure indicates a system dominated by an older stellar population, with limited evidence of ongoing star formation. There is no indication of spiral arms or prominent dust lanes. No signs of a recent or ongoing merger can be seen. The galaxy seems to be an isolated system.
