The galaxy presents a primarily smooth morphology with a slight ellipticity. It appears relatively undisturbed, with no readily apparent major mergers or tidal features. The color profile suggests a centrally concentrated population of older stars, exhibiting a yellowish-orange hue that transitions to a bluer, less intense color in the outer regions. This color gradient likely indicates a radial variation in stellar populations, with older, redder stars dominating the core and younger, bluer stars in the periphery. There is a slight hint of faint, diffuse disk-like structure, but it is not well-defined. Overall, the galaxy appears to be a massive system with a moderate star formation rate.
