The galaxy presents as an elongated structure, cigar-shaped in appearance. The light distribution suggests a relatively smooth profile, with a somewhat brighter central region transitioning to fainter edges. The color of the galaxy appears to be predominantly blueish, suggestive of a younger stellar population and potential ongoing star formation. There are no obviously resolved spiral arms or prominent dust lanes visible in the image, although a small amount of irregular and disturbed features can be seen, possibly indicating a minor interaction or merger event in its recent history. The galaxy's integrated light indicates an intermediate mass range.
