The galaxy appears to be a relatively small, elongated object. It exhibits a smooth light distribution, lacking prominent spiral arms or a distinct bulge. The galaxy's color profile suggests the presence of older stellar populations. There is a concentration of lighter, bluer light towards the center of the galaxy. The galaxy appears to have a low star formation rate, consistent with its overall color and smooth morphology. There are no signs of major disturbances or ongoing mergers; however, the cigar shape may indicate a possible past merger. 
