The galaxy appears to be a relatively smooth, elliptical structure with a concentrated central bulge. There is a discernible color gradient, shifting from a yellowish-white core to a redder outer halo. No distinct spiral arms or strong dust lanes are visible, suggesting a lack of significant ongoing star formation within a disk component. The galaxy presents a well-defined, rounded shape without apparent tidal disturbances or merging features. Overall, the morphology is indicative of an evolved galaxy dominated by an older stellar population.
