The galaxy presents as a generally smooth object, with an elliptical morphology appearing nearly round. There is a bright central bulge which diffuses outwards, with a subtle color gradient shifting from bluish near the center to slightly redder tones in the outer regions. Faint and indistinct features suggestive of spiral arms or a disk component might be present, but the resolution is insufficient to confirm this. There is no clear indication of significant ongoing star formation or major merger activity, though a slight asymmetry suggests possible minor interaction. The galaxy appears to be a relatively evolved system.