This galaxy presents as an elliptical structure, elongated in shape and exhibiting a smooth light distribution. There is minimal evidence of spiral arms or distinct features such as dust lanes. The galaxy has a yellowish-orange color gradient, indicating an older stellar population with a lack of recent star formation. There is a possible merging event occurring. This is indicated by the asymmetrical morphology. One lobe is larger than the other. The galaxy's diffuse halo fades smoothly into the background sky, suggesting no major tidal disturbances or interactions besides the possible minor merger taking place.