The galaxy presents as a well-defined elliptical morphology. It exhibits a smooth, centrally concentrated light profile with a high Sersic index, suggesting a dominant bulge component. The galaxy has a moderate axial ratio and a slight elongation. The color index indicates a relatively red population, implying older stellar populations and a suppressed star formation rate. No prominent dust lanes or spiral arm structures are discernible in the available image. There is no visible evidence of any major mergers or tidal disturbances. The lack of blue light further supports the conclusion of minimal recent star formation. The galaxy appears quiescent.
