The galaxy presents an elongated, cigar-shaped morphology. It exhibits a smooth light distribution, suggesting a relatively homogenous stellar population. There is a subtle hint of a central bulge, though it is not particularly prominent. The overall color is slightly redder, implying an older stellar population and reduced ongoing star formation. There might be a slight asymmetry or disturbance present, possibly indicating a past interaction or minor merger event, though the dominant impression is one of relative quiescence.
