The galaxy presents as an elliptical morphology. There appears to be a centrally concentrated bulge of high luminosity that occupies about half of the galaxy's visible profile. The outer regions of the galaxy gradually fade into the background sky, exhibiting a smooth light distribution with no apparent spiral arms or distinct features. Color gradients are subtle, with the central bulge tending toward redder hues while the outer regions showing slightly bluer tints, indicative of differences in stellar populations and age. There is no visible dust lane or active star-forming regions. The galaxy appears largely undisturbed.
