The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions into a more diffuse halo. The color gradient shows a distinct yellow to reddish hue in the central regions, suggestive of an older stellar population. Faint bluish tones are observed in the outer regions, potentially indicating some presence of younger stars or regions of on-going star formation, though limited. No prominent spiral arm structures or distinct dust lanes are visible. The galaxy's overall appearance is consistent with an early-type galaxy that has largely exhausted its supply of gas and dust for star formation. There appears to be little sign of major interaction or merger events influencing the galaxy's structure. The shape is highly rounded.
