The galaxy presents as a relatively smooth, elliptical-like structure with a moderate concentration of light toward the center. There is little evidence of spiral arms or a distinct disk. The color appears to be a yellowish-white, suggesting a population of older stars with lower star formation rate. The galaxy appears slightly elongated, but not heavily distorted. The overall appearance suggests a galaxy with a high mass and a low specific star formation rate, consistent with a relatively evolved system. There is a possible minor disturbance in its shape, indicative of a past or ongoing minor merger event.
