The galaxy appears to be a relatively smooth, centrally concentrated system. There is a notable radial color gradient, with the central region exhibiting a warmer, yellowish-white hue, potentially indicating an older stellar population. Surrounding this core, a bluer, more diffuse halo is visible, which may be indicative of recent or ongoing star formation, though at a low rate. The galaxy exhibits a mildly elliptical morphology, appearing to be neither perfectly spherical nor significantly elongated. No obvious signs of strong tidal disturbances or major merger activity are apparent, although there is some subtle asymmetry in the outer regions, possibly suggesting a minor interaction or past merger event. The overall structure suggests a transitioning galaxy, possibly evolving from a spiral towards an elliptical morphology.
