The galaxy presents as an elliptical morphology, exhibiting a generally smooth, diffuse light distribution. The central region appears brighter and more concentrated, indicative of a prominent galactic nucleus. A slight elongation is observed in the overall shape, suggesting a deviation from perfect sphericity. The color gradient transitions from a yellowish-white core to a bluer outer halo. There is no visual evidence of spiral arms, dust lanes, or significant star-forming regions. No major interactions or mergers are apparent.
