The galaxy presents a generally smooth, elliptical morphology. The central bulge is prominent, exhibiting a yellowish-white color, suggesting an older stellar population. Surrounding the core, a bluer, more diffuse halo is observed, hinting at ongoing, albeit moderate, star formation activity within the galaxy. While the dominant structure is smooth, a slight elongation is noticeable, deviating from a perfectly circular form, as well as some possible disturbances. Overall, the galaxy appears relatively isolated and is potentially in its later stage of development.