The galaxy presents a largely smooth and elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity moving outward. The galaxy appears largely homogenous in color, displaying a yellowish hue suggestive of an older stellar population. There is no clear evidence of spiral arms or significant dust lanes, indicating it is likely a mature system. There are no significant signs of ongoing merger activity or major disturbances in the overall structure. Overall, the galaxy appears to be an undisturbed elliptical galaxy with a relatively uniform stellar population and a high degree of central concentration.
