The galaxy presents as a relatively smooth, elongated structure with a subtle central bulge. It exhibits a blue-white color profile, suggesting the presence of a population of younger, hotter stars. The lack of prominent spiral arms or dust lanes indicates it is likely an early-type spiral galaxy or a lenticular galaxy, potentially undergoing a transition to a more quiescent state. There is a slight asymmetry to the outer regions of the galaxy, with a faint extension on one side, suggesting a possible minor interaction or tidal disturbance in its past.
