The galaxy appears to be a relatively smooth, centrally concentrated system. It presents a largely featureless morphology, with a dominant, luminous core that gradually fades into the outer regions. The galaxy exhibits an elliptical or lenticular shape, with a high degree of roundness, although subtle deviations from perfect circular symmetry are present. There's an indication of a faint, diffuse halo surrounding the central region, contributing to its overall extent. The color profile suggests a population of older stars, with a reddish hue, especially prominent toward the core. However, some bluer areas might suggest some degree of ongoing, though potentially low, star formation activity. There appear to be no signs of significant tidal disturbances or major mergers currently affecting the galaxy's morphology.
