The galaxy presents as a slightly elongated, disk-shaped structure. The central bulge is prominent and bright, exhibiting a smooth, concentrated luminosity. The disk component displays a subtle, almost indistinct spiral pattern. The color profile suggests a presence of both older stellar populations in the central bulge and relatively younger, bluer stars in the disk, even though there is no bright star formation obvious in the image. The galaxy shows no strong signs of active galactic nuclei activity or significant dust lanes. The galaxy's overall appearance is smooth and relatively undisturbed, consistent with an intermediate Sersic index, suggesting a morphological type between a pure elliptical and a spiral galaxy.
