The galaxy appears as a centrally concentrated, elliptical-like object with a generally smooth morphology. The core exhibits a bright, intense yellow hue, suggesting a high concentration of older stellar populations. There's a gradual decrease in brightness moving outward from the core, with the outer regions fading into a more diffuse, greenish halo. No distinct spiral arms or disk-like structures are discernible, and the galaxy exhibits a largely undisturbed, relaxed appearance. Slight irregularities in the outer halo may indicate a low level of past or ongoing interaction, but no major merger events are immediately apparent. The overall color profile suggests that star formation is relatively low.
