The galaxy presents as a single, fairly uniform object with a smooth, elliptical morphology. It appears highly concentrated with a bright central bulge, indicating a relatively old stellar population dominating the core. The color profile shifts from yellow-orange in the center to a slightly redder hue in the outer regions. No distinct spiral arms or significant dust lanes are apparent. There is a subtle suggestion of an extended halo surrounding the main body, which appears diffuse and faint. The overall structure suggests a galaxy that is well-evolved and potentially quiescent in terms of star formation activity.
