The galaxy presents a generally smooth, elliptical morphology. The core is relatively bright and concentrated, indicating a high density of stars in the central region. There is a subtle color gradient, appearing slightly bluer in the outermost regions compared to the yellowish core. This could indicate younger stellar populations in the outer areas, potentially with ongoing star formation. The overall round shape suggests a system dominated by random stellar motions rather than organized rotation, typical of elliptical galaxies. There is no apparent evidence of spiral arms or a prominent disk component. Faint disturbances or tidal features are not clearly visible, suggesting the galaxy is not currently undergoing a major merging event. The galaxy's spatial extent is moderate, appearing neither overly compact nor excessively diffuse. Based on the color and morphology, this galaxy is likely a mature system.
