The galaxy presents as a relatively smooth, elliptical-like structure with a noticeable concentration of light toward the center. The light profile appears centrally concentrated, suggesting a well-defined nucleus. The overall color is yellowish, which is characteristic of an older stellar population and reduced star formation. There is little evidence of spiral arms or significant dust lanes, supporting the classification as a galaxy lacking prominent disk features. Faint blue light is evident in the outer regions, which could be indicative of a small amount of recent or ongoing star formation, even if the rate is quite low relative to its mass. There is a slight deviation from perfect roundness, being more elliptical in shape. The galaxy does not appear to be undergoing any major merging events or show signs of significant tidal disturbances, although there may be slight irregularity at the edge of the visible region. The overall impression is that of a massive galaxy that has largely exhausted its supply of gas for star formation and has been evolving passively.
