The galaxy presents as an elliptical or lenticular type with a dominant smooth morphology. It exhibits a centrally concentrated light profile, suggesting an older stellar population. A slight elongation is observed, but it is generally round in appearance. The color is predominantly yellow-orange, indicative of a lack of significant ongoing star formation. There are no clearly defined spiral arms or dust lanes visible. A faint, diffuse halo may be present surrounding the main galactic body. There is no strong evidence of a major merger event, although some minor asymmetries or disturbances cannot be entirely ruled out given the image resolution.
