The galaxy presents as an elongated, cigar-shaped structure with a smooth, relatively featureless morphology. The light distribution suggests a significant spheroidal component, and there is a yellowish hue in the central region, indicative of an older stellar population, likely concentrated in a bulge. The galaxy extends outwards with fainter bluish light, suggestive of younger, star-forming regions in a disk. There is no strong indication of spiral arms, although the shape suggests a disk-like structure. Minor irregularities in the outer light distribution may hint at past interactions.
