The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth morphology with a high degree of central concentration. The primary color appears yellowish, suggesting a population of older stars and a relatively low star formation rate. The galaxy appears round with a high concentration of old stars in the core of the galaxy. There is a small amount of what appears to be dust, potentially. There is no evidence of major recent mergers or tidal disturbances. The object displays an overall homogenous structure without pronounced spiral arms or a distinct disk.
