The galaxy presents a smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a bright, nearly unresolved core that gradually fades into an extended halo. The color profile suggests an older stellar population, as indicated by the redder hues concentrated toward the core, transitioning to slightly bluer tones in the outer regions, possibly reflecting the presence of younger, though likely still subdued, star formation in the disk. There appears to be a slight asymmetry in the outer isophotes, suggesting the possibility of a past minor interaction or tidal disturbance, though no distinct merging features are readily apparent. The overall structure suggests a galaxy that has largely completed its merging history and is currently evolving passively.
