The galaxy presents as a largely smooth, elliptical-like object with a bright central bulge, and is approximately 6.5 kpc in radius. The light distribution is centrally concentrated, and overall, it appears relatively undisturbed, showing no significant signs of ongoing merger activity. There is a slight hint of bluer light in the outer regions of the disk, which may indicate the presence of some star formation, although at a low rate. The overall color of the galaxy is relatively red, suggesting a population of older stars dominating the light output.
