The galaxy presents as a centrally concentrated, relatively smooth elliptical or lenticular structure. There is a dominant bulge component exhibiting a yellowish hue, possibly indicating an older stellar population with reduced recent star formation. The outer regions appear more diffuse and display subtle blue tones, suggesting the presence of a younger stellar population. The galaxy is generally round. There appears to be no strong evidence of major tidal disturbances or ongoing mergers, although minor asymmetries cannot be ruled out at this resolution. Overall, the galaxy exhibits characteristics consistent with a relatively evolved system.