The galaxy presents as a concentrated elliptical, exhibiting a centrally-dominant bulge. The light distribution is smooth and generally symmetrical, showing a slight elongation. The core of the galaxy exhibits a yellow-orange hue, with color gradients suggesting a population of older stars. There is minimal evidence of spiral arms, strong dust lanes, or ongoing star formation. The outer regions of the galaxy fade gradually into the background. There is a slight hint of tidal disturbance or a minor companion influencing its shape. Overall the object is a large and old, with a small amount of active star formation.
