The galaxy presents a largely smooth morphology, exhibiting a centrally concentrated spheroid shape. The galaxy's core appears yellow-orange, suggesting a dominant population of older stars. Fainter, greenish hues are observed in the surrounding regions of the galaxy, which may imply ongoing, but limited, star formation activity. A significant portion of the galaxy appears undisturbed, with no signs of significant tidal features or ongoing merger events. The galaxy is not perfectly circular, but its shape does suggest an overall elliptical classification.
