The galaxy presents a largely smooth, elliptical morphology, with little to no visible disk structure. It exhibits a bright, concentrated central bulge that gradually fades into the outer regions. The overall color appears to be yellowish-orange, suggesting a population of older stars with minimal ongoing star formation. No distinct spiral arms or dust lanes are apparent. The galaxy appears to be relatively isolated, showing no obvious signs of interaction or tidal disturbances from neighboring galaxies, maintaining a generally relaxed structure. Its round shape may indicate it is viewed close to face-on, exhibiting a symmetrical and undisturbed formation. The absence of blue color components suggests a low rate of star formation within the galaxy.
