The galaxy presents as a somewhat elongated structure, approximately 9 kpc across. Its morphology is generally smooth, although there appears to be some minor asymmetry or disturbance in its form. The light distribution suggests a centralized concentration, possibly a bulge component, surrounded by a more diffuse halo. The overall color is relatively red, indicating an older stellar population or significant dust obscuration, potentially suppressing bluer wavelengths. There is no clear evidence of spiral arms or active star formation regions visible in this image. The galaxy's shape appears to be somewhere between round and cigar-shaped. There isn't any indication of a recent or ongoing major merger.
