The galaxy presents as a diffuse, extended object exhibiting a somewhat irregular morphology. The light distribution is not centrally concentrated; instead, the galaxy appears as a collection of fainter, overlapping regions. There is evidence of some distortion. The color distribution indicates variations across the galaxy, with areas showing bluer tones and others showing redder tones. The overall color is slightly red, indicating older star populations or substantial dust extinction. The galaxy's structure does not indicate a clear spiral arm pattern or a well-defined elliptical shape. The galaxy seems disturbed.
