The galaxy presents a smooth, elliptical morphology, with a slightly elongated profile. The color gradient suggests a redder core, potentially indicating an older stellar population concentrated towards the galactic center. There is little evidence of spiral arms or significant dust lanes within this particular image. Overall, the galaxy appears to be relatively undisturbed, displaying a lack of significant tidal features or ongoing merger activity. The galaxy appears to be relatively distant, given the faintness of the light.
