This galaxy appears to be a relatively compact and luminous object. Its morphology is largely smooth, with a somewhat elliptical shape and a high degree of central concentration. The light distribution suggests a dominant bulge component. There is a possible presence of faint extended features or a very diffuse disk, though they are not prominent. There is a slight color gradient visible, with the central region exhibiting a bluer hue compared to the outer regions, which are slightly redder. No prominent spiral arms or dust lanes are observed. There may be evidence of faint tidal features or minor disturbances indicating a possible minor merger in its history, although no major disturbance can be seen.
