This galaxy exhibits a generally smooth morphology, with a high degree of central concentration. It appears nearly round in shape. There is a very slight indication of some disk-like structure. The galaxy exhibits a color gradient, becoming slightly redder towards the center. There is no clear evidence of a major ongoing merger or significant tidal disturbances, but there appears to be a hint of minor irregularity. The low star formation rate suggests it is most likely an older galaxy. The galaxy's estimated size is around 2 kpc in radius, making it a relatively small galaxy.
