The galaxy exhibits a distinct spiral structure. Two prominent spiral arms are clearly visible, tightly wound around the central bulge. The arms display a clumpy texture, suggestive of active star formation regions. The central bulge is of moderate size, appearing bright and somewhat smooth, likely populated by older stellar populations. There is no obvious bar structure bisecting the bulge. The disk is observed nearly face-on. No major mergers or tidal disturbances are readily apparent, though a minor asymmetry in one of the spiral arms may indicate a past interaction. The galaxy appears to be in a relatively quiescent state.
