The galaxy presents as a relatively smooth, centrally concentrated object. The color profile suggests an elliptical morphology with a likely older stellar population. There is a very faint, diffuse disk component that surrounds the central bulge. No spiral arm structures are discernible. The galaxy shows a slight elongation and is more disk-like than it is round. There is no visually apparent ongoing major merger activity or significant tidal disturbances. A very slight asymmetry is present, and the blue color suggests some star formation.
