This galaxy presents as a relatively smooth, elliptical structure. The light profile appears centrally concentrated with a gradual falloff in intensity towards the outer regions, though this is difficult to ascertain given image resolution. The color indices suggest a redder overall color, indicating an older stellar population with less ongoing star formation. No spiral arms or distinct features such as dust lanes are readily apparent, which is consistent with an elliptical morphology. Given its apparent smoothness and color, this galaxy likely has a significant mass. There is no evidence of any ongoing major merging activity or significant tidal disturbances. The morphology suggests it is likely a relaxed system that has undergone significant internal processing and is in a relatively stable state.
