The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The light distribution suggests an older stellar population, with a lack of prominent spiral arms or active star-forming regions. The galaxy is slightly elongated, with a round-to-in-between shape. There is no obvious evidence of an ongoing merger, although some minor tidal disturbances cannot be completely ruled out. Its color profile indicates a redder hue, consistent with a redshift of approximately 0.17, suggesting that this is a relatively distant galaxy. Based on the characteristics observed, the object likely possesses a significant stellar mass.
