The galaxy presents a predominantly smooth and rounded morphology, suggesting an elliptical or lenticular classification. Its color appears largely homogenous, with a central concentration of yellowish-white light that fades into a greenish-yellow hue towards the outer regions. A subtle, diffuse disk feature might be present, though not sharply defined. There appears to be little to no evidence of spiral arm structure, strong dust lanes, or active star-forming regions. The overall structure lacks signs of ongoing major mergers or significant tidal disturbances, with a possibility of only minor disturbances to its structure. The galaxy exhibits a generally quiescent nature, with a smooth and evolved stellar population dominating its light output.
