The galaxy presents an elongated, cigar-shaped morphology. The light profile appears relatively smooth, although some subtle features may be present. A central bulge region shows increased luminosity, with the galaxy fading into a broader disk. Color gradients suggest the possibility of an aging stellar population. The galaxy's light is shifted to the redder portion of the spectrum, which would make sense if it is far away. There may also be a minor disturbance occurring. The general symmetry of the overall structure does not give reason to suggest a major interaction.