The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy, exhibiting a centrally concentrated bulge. The light distribution is fairly uniform without prominent spiral arm structures. There is a slight elongation but it mostly appears round. The galaxy displays a color gradient, with the central region appearing more yellow in color. The outer regions have less luminosity and appear less colored, which may indicate the presence of an older stellar population and a lower rate of current star formation activity. There is no obvious indication of ongoing merging events or major disturbances in the galaxy's overall morphology.
