The galaxy presents as a somewhat elliptical, relatively smooth object. Its core exhibits a bright, concentrated luminosity that fades outward into a more diffuse halo. There is a slight elongation, though it is predominantly round in appearance. No distinct spiral arm structures are discernible within the visible spectrum. The overall color profile indicates a population dominated by older stars, trending towards the redder end of the spectrum, though with some contributions from bluer wavelengths in the surrounding areas. There is some subtle evidence of a minor disturbance in its overall symmetry but the overall morphology suggests a quiescent or post-starburst galaxy. Evidence for mergers are slight. 
