The galaxy presents a generally smooth morphology, with a centrally concentrated light profile. It exhibits a predominantly elliptical shape, appearing nearly round. The color profile suggests a relatively evolved stellar population. While the galaxy appears mostly uniform, there might be a very subtle indication of a faint, diffuse disk-like component oriented along the major axis, but this is highly uncertain. There's no obvious indication of recent or ongoing major merger activity, tidal tails, or strong morphological disturbances. The overall appearance suggests a system with a significant bulge component, and the integrated luminosity hints at a substantial mass. The color suggests an older stellar population with ongoing star formation.
