The galaxy presents as an elongated, cigar-shaped structure. It exhibits a relatively smooth and featureless morphology, appearing mostly homogeneous across its body. The light distribution suggests a concentration of older stellar populations, producing a redder hue, though some regions show a hint of bluer light perhaps indicating a low level of on-going star formation. There is no clear evidence of spiral arms or a central bulge. The overall appearance does not suggest any significant tidal disturbances or mergers.
