The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, concentrated morphology with no distinct spiral arm structure apparent in the image. The light distribution appears generally symmetrical. The galaxy displays a strong central bulge, characterized by a yellowish-orange color, suggesting a high population of older stars. The outer regions of the galaxy fade gradually into the background sky, with a subtle halo of light. The overall color indicates a galaxy with reduced recent star formation activity and an older stellar population. There may be a hint of subtle tidal features or disturbances, but it is difficult to assess any recent merger or interaction.