The galaxy appears as a centrally concentrated system with a smooth, elliptical morphology. The color profile is primarily yellow-orange, indicative of an older stellar population. There is a subtle color gradient from the core outward, with the central region appearing slightly more yellow than the surrounding halo. The galaxy presents a relatively high degree of symmetry, with no apparent spiral arm structures or prominent dust lanes visible in this imaging. The general morphology suggests an evolved system, possibly a lenticular or elliptical galaxy, with a relatively quiescent star formation rate.
