This galaxy exhibits a generally elliptical morphology, appearing mostly smooth with minimal discernible disk structure. The light distribution suggests a centrally concentrated spheroid, possibly an elliptical galaxy, with decreasing luminosity outward. The galaxy has a yellow-red hue centrally, transitioning to a bluer color toward the edges. This color gradient could indicate a shift in stellar populations, with older, redder stars dominating the core and younger, bluer stars populating the outer regions. There is a hint of possible minor tidal disturbances, as indicated by slight asymmetries in the outer light distribution. The relatively smooth appearance indicates that it has either completed a major merger, or no major merger has occurred recently.
