The galaxy presents a predominantly smooth morphology, indicative of an elliptical or lenticular type. A slight elongation is observed along its major axis, suggesting a deviation from perfect sphericity, but it is close to round. The galaxy exhibits a central bulge that appears as a concentrated region of high luminosity. The color gradient transitions from a yellowish-white core to a more reddish hue in the outer regions. This color difference likely indicates older stellar populations dominating the outer regions, while the inner regions have slightly younger populations. There is no clear evidence of spiral arm structures or significant dust lanes. No signs of active galactic nuclei activity is present. 
