The galaxy presents as a somewhat diffuse object with a concentrated central region. It exhibits a primarily smooth morphology, with a degree of ellipticity, appearing neither perfectly round nor highly elongated. There are subtle color gradients visible, suggesting a slightly bluer central region and a redder outer halo. The galaxy's overall structure appears relatively undisturbed. There is no evidence of strong tidal features or ongoing major mergers. Overall, it has a weak indication of a spiral structure or disk component, but the resolution is limited.
