The galaxy presents a generally smooth morphology with minimal discernible features. It is largely elliptical in shape, exhibiting a high degree of roundness. The galaxy's light profile appears centrally concentrated with a bright core, suggesting a possible supermassive black hole at its center. The color gradient transitions smoothly from a yellowish-white central region to a bluer hue towards the outer edges, indicative of a declining population of older stars in the core and pockets of younger star formation activity in the outer regions, albeit at a relatively low rate. No evidence of major mergers or significant tidal disturbances is apparent; however, the galaxy may be experiencing minor disturbances.
