The galaxy exhibits a flattened, elliptical morphology. It has a generally smooth appearance with a high degree of central concentration. The galaxy displays a core of yellowish-white hue, surrounded by a more diffuse, bluish outer region. The color gradient from the center to the edge suggests a potential transition in stellar populations, with older, redder stars dominating the core and younger, bluer stars contributing to the outer regions. There are no distinct spiral arm structures or significant dust lanes visible. The lack of these features points towards a likely early-type galaxy classification.