The galaxy presents as a centrally concentrated object, with a high degree of smoothness observed in its overall structure. It appears slightly elongated, displaying an intermediate ellipticity. No prominent spiral arm structures or dust lanes are discernible. The light profile suggests a radial decrease in surface brightness from the core. There is a hint of an extended halo surrounding the central bulge. Interactions with nearby galaxies do not seem apparent as there are no tidal tails or distorted morphological features. The color is fairly uniform, although the central region appears slightly bluer than the outer regions. The galaxy appears quiescent with only a small amount of star formation.
