The galaxy presents as a disk-shaped system, viewed at a significant inclination. A bright central bulge is evident, with a somewhat diffuse appearance. The disk component exhibits a color gradient, appearing bluer towards the outer regions, suggestive of ongoing star formation. The overall structure is relatively smooth, with only subtle indications of spiral arm structure or prominent dust lanes. There are possible indications of a minor disturbance in the galactic structure, but overall the structure appears to be mostly undisturbed. The angular size suggests a physically large galaxy, and the luminosity indicates a substantial stellar population.
