The galaxy presents as a centrally concentrated, luminous object with a generally smooth appearance. The light profile suggests a relatively high degree of symmetry and ellipticity appears low, possibly tending toward a more spheroidal morphology. There may be a faint disk. The central region exhibits a higher intensity in g, r, and z bands suggesting a high concentration of older stars. The overall color gradient suggests a galaxy that is no longer vigorously forming stars in its outer regions, with lower intensity g, r, and z bands there. There are hints of some minor disturbances or asymmetries in the outer edges of the galaxy, indicating possible interactions. There are some faint, blueish streaks in the outer areas.
