The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth, featureless morphology. The light distribution appears centrally concentrated with a radial falloff, and the shape appears moderately round. There is no distinct disk structure visible and no indication of significant spiral arms or prominent dust lanes. 

The galaxy appears to be experiencing minimal current star formation activity. There is evidence of a possible minor disturbance to the galaxy, although there are no major visual indicators of a recent or ongoing merger. The overall appearance suggests a relatively evolved system with a substantial mass. The galaxy is emitting strongly in the redder parts of the spectrum. 
