The galaxy appears to be a relatively compact system at a redshift of approximately 0.156, indicating it is at a considerable cosmological distance. Morphologically, it presents a smooth, elliptical appearance, with a high degree of roundness. There is no strong evidence of spiral arm structure, though the image quality is limited.

The galaxy exhibits a concentrated central bulge region. The overall color profile suggests an evolved stellar population, likely dominated by older, redder stars, though a small amount of bluer light is present. The star formation rate appears low, consistent with a galaxy that has largely exhausted its gas supply. There is evidence of possible disturbances indicating that it might be in the process of merging with another galaxy.
