The galaxy presents as a luminous elliptical or lenticular type, appearing generally smooth in texture. There is a highly concentrated bulge in the center of the galaxy, indicated by the increased luminosity in the center. The isophotes are closely packed and the object appears roundish, though slightly elongated. There is a faint indication of spiral arm structure. The luminosity profile suggests a single component system with a centrally dominant elliptical bulge. The galaxy exhibits an absence of strong spiral arms or dust lanes. The color gradient indicates a higher concentration of older stellar populations, with an extremely low star formation rate within the system. There is a minor tidal disturbance. Overall, this appears to be a red and relatively quiescent galaxy.
