The galaxy presents as a slightly elongated, elliptical structure. It displays a largely smooth morphology with a dominant central bulge exhibiting a yellow-red hue, suggesting an older stellar population. There appears to be a faint disk, almost edge-on, but not sharply defined. There are no prominent spiral arms visible. There might be some minor disturbances in the structure suggesting a previous or ongoing minor interaction. The concentration of light is higher in the center. Overall, the galaxy seems relatively isolated with a somewhat symmetrical shape.
