This galaxy exhibits a smooth morphology, appearing largely featureless in the available image. It has an elongated, cigar-like shape. The light distribution is relatively uniform, with a slightly brighter central region that is not sharply defined as a bulge. The galaxy displays a blueish hue, potentially indicating the presence of relatively young stellar populations. There is no obvious dust lane or spiral arm structure visible. The lack of visible disturbances suggests that it is likely not undergoing a major merger event.
