The galaxy appears to be elliptical in shape, exhibiting a generally smooth morphology with a high degree of roundness. It presents a yellowish-orange hue, which might be indicative of an older stellar population with a lower rate of active star formation. There is little to no evidence of distinct spiral arm structures or significant dust lanes. A subtle color gradient is observed, suggesting a possible concentration of older stars towards the core. Minimal signs of tidal disturbances or ongoing merger activity are apparent; the galaxy appears relatively undisturbed.
