The galaxy presents as a relatively smooth, centrally concentrated object with a high degree of radial symmetry. It appears largely elliptical in shape. The light distribution suggests a prominent bulge component, characterized by a bright, diffuse glow that dominates the galaxy's core.  The overall color appears to be on the redder end of the spectrum. There is minimal evidence of distinct spiral arms or prominent dust lanes within the galactic disk. The galaxy exhibits a notable absence of bright, blue star-forming regions. There may be some very subtle disturbances indicating minor interaction with another galaxy.
