The galaxy presents as an elongated, relatively smooth object with a somewhat cigar-shaped morphology. The light distribution appears centrally concentrated, suggesting a higher stellar density towards the center of the galaxy. It exhibits a blueish-white hue, potentially indicating the presence of younger stellar populations. The galaxy displays a generally undisturbed structure, without apparent signs of major merging activity, although the faintness of the outer regions limits a full morphological assessment. 
