The galaxy appears as a single, relatively smooth structure, suggesting an elliptical morphology. It exhibits a concentrated central bulge that fades gradually toward the edges. The color profile is predominantly yellowish-orange, indicating an older stellar population with a lack of significant ongoing star formation. The elongated shape suggests some degree of rotational support. There are no readily apparent signs of spiral arms, dust lanes, or recent major merger events, and the overall undisturbed morphology may indicate a relatively quiescent evolutionary history. The angular size implies that it is a moderately large galaxy.
