The galaxy presents as a predominantly smooth, centrally concentrated object. Its color profile is dominated by yellow hues, with subtle hints of redder tones apparent in the outer regions. No distinct spiral arm structures or prominent dust lanes are visible. The overall morphology suggests an elliptical or lenticular galaxy type, with a high degree of sphericity. The light distribution appears relatively uniform, indicative of a well-mixed stellar population. There is no obvious evidence of ongoing major merger activity or significant tidal disturbances.
