The galaxy presents a primarily smooth, elliptical morphology. It exhibits a bright, concentrated central bulge with a yellowish hue, indicating a population of older stars. A subtle, diffuse disk surrounds the bulge, showing a slight flattening and a hint of blueish tones, potentially indicating some ongoing star formation. There appears to be a very slight disturbance to the symmetry, possibly a minor tidal interaction or internal kinematic effect. No prominent spiral arms or bar structures are discernible. Overall, the galaxy appears relatively undisturbed and evolved.
