The object presents as a galaxy with a redshift of approximately 0.139. Morphologically, it appears largely smooth, lacking prominent spiral arms or a distinct disk structure. The galaxy exhibits an elliptical shape, tending towards roundness but predominantly in an intermediate classification between round and elongated. There is no visually apparent major disturbance or ongoing merger event, however a small disturbance can not be ruled out. Photometrically, the galaxy shows decreasing magnitude values from g-band to z-band, indicating a redder color. Overall, the galaxy appears to be a relatively massive system with a low ongoing star formation rate.
