The galaxy presents as a somewhat elliptical, moderately luminous system. It exhibits a smooth, centrally concentrated light profile, indicative of an early-type galaxy morphology. There is minimal evidence of spiral arm structure or prominent dust lanes. The galaxy's color appears to be a relatively uniform blue-white, suggesting the presence of a moderate population of younger stars, but overall it is composed of an older stellar population. There appears to be a faint tidal stream or distorted halo, suggesting that it might have undergone a minor merger event in the past. Overall, the galaxy exhibits properties consistent with either an elliptical galaxy or a lenticular galaxy seen at an oblique angle. The relatively small apparent size and uniform color suggests that star formation rate is slow compared to the total stellar mass.
