The galaxy presents as a relatively small, elongated object with a smooth, diffuse morphology. Its overall shape is cigar-like, lacking any obvious spiral arms or significant substructure. A central bulge is difficult to discern, suggesting a more flattened, disk-dominated system. The light distribution is brightest in the central region, fading gradually towards the edges. The color appears to be a relatively even blue-white, which indicates the presence of a young population of stars. There is no evidence of any major ongoing mergers or tidal disturbances.
