The galaxy presents as a somewhat compact structure with a generally elliptical morphology, though with hints of asymmetry and some distortion. Its light profile appears relatively smooth. There's a central concentration of light suggesting a bulge or nucleus, with luminosity decreasing gradually outward. There are no prominent spiral arms or distinct bar structures visible, indicating a probable classification as an elliptical or lenticular galaxy. There is a hint of minor disturbance in the surrounding area. The galaxy appears to be composed of an older stellar population as indicated by its redder color. There is potential for a merger event, past or future, to be affecting this galaxy. There appears to be an estimated effective radius of approximately 10 kpc.
