The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be elliptical in shape, exhibiting a high degree of roundness. There is little evidence of spiral arm structures or significant dust lanes. The light distribution suggests a central bulge that dominates the galaxy's overall luminosity. A faint, diffuse halo extends outwards from the central region. The galaxy appears relatively undisturbed, with no obvious signs of ongoing or recent major mergers. The galaxy's color suggests a moderate amount of star formation.
