The galaxy presents as a slightly elongated, centrally concentrated system. It exhibits a relatively smooth morphology, with a diffuse halo surrounding a brighter central region. The light distribution suggests an elliptical or lenticular galaxy type, with a significant bulge component. The color appears relatively uniform across the galaxy, with a hint of redder hues, possibly indicating an older stellar population. There is no discernible spiral arm structure or active star-forming regions. The galaxy shows no signs of major disturbances or tidal features, suggesting that it may be a relatively settled system. 
