The galaxy presents as a smooth, elliptical-like structure with a centrally concentrated brightness profile. It exhibits a yellowish-white hue, suggesting an older stellar population. The overall form is quite regular with no immediately apparent features, such as spiral arms or prominent dust lanes. There is a subtle color gradient observable, with the central region appearing slightly more yellow, while the outer halo demonstrates a hint of bluer tones. The light is concentrated with no evidence of merging or tidal tails, indicating that it is unlikely to be experiencing major interactions.
