The galaxy presents as a lenticular, or potentially spiral, system with an estimated diameter of approximately 5.4 kpc. The overall color is bluish, suggesting the presence of younger stellar populations and ongoing star formation, albeit at a moderate rate. The light is distributed smoothly across the central region with a moderate amount of visible disk structure, and is elongated in shape, appearing cigar shaped. There is a clear absence of significant dust lanes or pronounced spiral arm structures. There may be a small dwarf galaxy in close proximity to the main galaxy. There is no visual evidence of any major interactions or merger events, although there are some signs of minor disturbances.
