The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge and a more diffuse halo. It is generally round in appearance, exhibiting a subtle elongation. There is little evidence of prominent spiral arms or significant dust lanes. The galaxy displays a color gradient, appearing bluer in the central regions and redder toward the outer edges of the halo, which could indicate a difference in stellar populations, with younger, hotter stars concentrated in the center. There is some evidence of minor disturbances in the outer regions, but no signs of a major merger event. The stellar mass of this galaxy is relatively high, but its star formation rate appears suppressed.
