The galaxy presents an overall elliptical morphology, with a smooth, concentrated light distribution. The color indices suggest a galaxy dominated by an older stellar population, with a redder color indicative of lower recent star formation. There appears to be no clear evidence of spiral arms or a prominent disk structure. The isophotes appear relatively undisturbed, lacking significant tidal features, close companion galaxies, or major distortions. The galaxy exhibits a fairly round appearance. There may be a slight asymmetry in the light distribution, potentially indicating a minor interaction or past merger event, but overall the galaxy appears largely relaxed and undisturbed. Its luminosity suggests it is a relatively massive system.
