The galaxy appears to be an elliptical galaxy with a smooth, diffuse light distribution. There is a distinct central bulge which is more yellow in color, possibly indicating an older stellar population. The outer regions of the galaxy are more blueish, indicating the presence of younger stars or low levels of ongoing star formation. The overall shape is fairly round, with no clear evidence of spiral arms or a distinct disk structure. There may be some minor disturbances or asymmetries in the outer halo, but no major merging activity is apparent. The galaxy seems relatively isolated in the field.
