The galaxy presents as an intermediate object, neither a pure elliptical nor a well-defined spiral. It exhibits a degree of smoothness, with a somewhat amorphous structure. A slight elongation is observed, but it does not appear highly flattened or cigar-shaped. Evidence suggests potential interaction or disturbance, although not a major merger. The presence of both bluer and redder regions indicates mixed stellar populations. The galaxy likely possesses a moderate mass. Observed colors suggest it has some on-going star formation, though perhaps at a moderate or low rate for its mass.
