The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated luminosity profile. It displays a generally rounded morphology, though its ellipticity is noticeable. The core exhibits a yellowish-white hue, potentially indicating an older stellar population with a higher concentration of evolved stars. Moving outwards from the core, the color shifts slightly to a bluer tint, suggesting the presence of some younger stars. There is no distinct spiral arm structure visible. Subtle, irregular features hint at a possible minor disturbance or interaction, but the overall structure is predominantly smooth. Star formation is likely present at a low to moderate level, as indicated by the color gradient within the galaxy. 
