The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge with a somewhat diffuse halo. The overall color appears to be yellowish-red, suggesting a population of older stars, with possible dust obscuration. There is no clear evidence of spiral arms or significant star formation regions within the visible light spectrum. The galaxy appears to be isolated, showing no signs of major tidal disturbances or ongoing mergers with other galaxies. The morphology suggests an evolved system with a quiescent star formation rate.
