The observed galaxy presents as a roughly circular, indistinct luminous object. The overall structure appears to be fairly smooth, lacking strong spiral arms or prominent features usually indicative of active star formation regions. The light emitted is generally uniform, with only very subtle variations in intensity across the galaxy's disk. Based on the faintness of the galaxy and apparent lack of significant features, there are no obvious signs of a recent major merger or significant tidal interaction. The overall morphology suggests this is a relatively mature galaxy. Possible minor disturbance or slight asymmetry may be present but the features are indistinct.
