The galaxy presents a generally smooth, elliptical morphology, exhibiting a somewhat elongated shape. A central bulge dominates the galaxy's structure, appearing bright and yellowish-white, potentially indicating a higher concentration of older stellar populations. Fainter, bluish light extends from the central region in a diffuse manner, possibly indicative of a weak disk or extended halo where some star formation may be occurring. There are no apparent spiral arm structures or significant dust lanes visible. Overall, the galaxy appears relatively undisturbed, with no obvious signs of a major ongoing merger. There might be a subtle asymmetry or minor perturbation, but this would need to be verified with deeper data.
