The galaxy appears to be a faint, diffuse object, exhibiting a somewhat elongated morphology. The light distribution is not uniform, showing a subtle central concentration. There are no apparent spiral arms or distinct disk structures visible. The overall color suggests a redder spectral energy distribution, potentially indicating an older stellar population or significant dust obscuration. The galaxy's profile does not suggest a perfectly elliptical or spherical shape. There are subtle signs of irregularities in the galaxy's structure which suggests some potential tidal disturbances in its past, although no major merger is evident. The galaxy is not perfectly smooth, and shows some features.
