The galaxy presents as an elliptical-like system, exhibiting a smooth, concentrated light profile. It appears largely featureless, with no readily discernible spiral arms or distinct structures. The central region is characterized by a brighter, more intense luminosity, suggesting a concentration of older stellar populations or perhaps a low-luminosity active galactic nucleus. A diffuse halo surrounds the central core, fading into the background sky. The object displays a slight elongation, deviating marginally from a perfect circular shape. There is no immediate visual evidence of significant ongoing mergers or major tidal disturbances. Its color appears relatively red, indicative of a population of evolved stars and a reduced rate of star formation.
