The galaxy presents an overall elliptical morphology, appearing largely smooth with a high degree of central concentration. The color gradient suggests a bluer core region that transitions to redder hues in the outer regions. There is no apparent spiral structure or distinct features such as prominent dust lanes or tidal tails, suggestive of minimal recent merger activity or strong interactions with neighboring galaxies. Its smooth, featureless appearance is likely due to the old stellar populations that dominate its composition.
