The galaxy presents as a largely featureless elliptical or lenticular system. It exhibits a high degree of central concentration, with a bright core that gradually fades into the surrounding galactic halo. The halo appears smooth and relatively uniform, with only a subtle ellipticity. There is no evidence of prominent spiral arms or a well-defined disk structure. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or ongoing mergers with nearby galaxies, although there may be a minor disturbance to the overall shape. Based on color indices, star formation is likely suppressed within the galaxy. The dominant stellar population appears to be older and redder, indicative of evolved stars. The galaxy appears quite round with no cigar-like shape.
