The galaxy presents a generally smooth morphology, with approximately 90% of citizen scientists who reviewed the image noting this. The light distribution is fairly even and centralized. It has a subtle degree of elongation and, while most appear to think its shape is "in between", it has a bias toward roundness rather than appearing as a highly elongated or cigar-shaped galaxy. No prominent spiral arms, bars, or other major features are visible. There is no indication of ongoing major or minor mergers, as evidenced by the absence of tidal tails, bridges, or other obvious signs of disturbance in its overall form. There is the possibility of some star formation activity, though without further data on emission lines, a conclusive determination is not possible. The galaxy appears to have a redder color, indicating it may be composed of an older stellar population.
