This galaxy presents as a centrally concentrated object, exhibiting a generally smooth morphology. The light distribution suggests a significant spheroidal component, potentially indicative of an elliptical or lenticular galaxy. While a disk component might be present, it does not appear prominent within the image. The overall color profile leans towards the redder end of the spectrum, hinting at an older stellar population and relatively low ongoing star formation. There's no clear evidence of strong tidal features or major disturbances, although there may be some minor asymmetries in the outer regions of the halo suggesting there could have been a minor interaction with another galaxy at some point in the past.
