The galaxy presents as a somewhat amorphous, centrally concentrated object. It exhibits a smooth, elliptical morphology, displaying a gradual decrease in luminosity from the core outwards. The galaxy’s color appears to be a blend, with a warmer, yellowish hue concentrated within the central bulge, transitioning to cooler, bluish tones in the outer regions. This suggests the potential presence of an older stellar population dominating the core, with younger, bluer stars contributing to the outer halo. No distinct spiral arm structures or dust lanes are apparent within this image, suggesting that star formation may be occurring at a low rate. The overall structure and color profile suggest a fairly evolved galaxy, potentially undergoing passive evolution. There is a small object that could be tidal debris suggesting a past merger event, which is consistent with minor disturbances.
