The galaxy presents an elongated, cigar-shaped morphology. It exhibits a smooth overall structure, lacking distinct spiral arms or a prominent central bulge. The core of the galaxy appears brighter and more concentrated, with a yellowish-white hue, potentially indicative of an older stellar population. Fainter blue-ish regions are observed towards the periphery of the galaxy, perhaps suggesting pockets of more recent star formation. No significant tidal features or signs of recent mergers are clearly discernible in the image. The light distribution gradually fades outwards from the central region, giving the galaxy a somewhat diffuse appearance. There does not appear to be a significant dust lane present.
