The galaxy presents a largely elliptical morphology. The light distribution appears smooth and centrally concentrated, with a minor axis ratio suggesting a nearly round shape. There is no obvious evidence of spiral arm structures or a prominent disk. The galaxy exhibits a relatively uniform color gradient, indicating a lack of ongoing major star formation. Faint, diffuse light extends outward from the central region, gradually fading into the background. No strong tidal features or indications of recent major merger activity are apparent, though slight asymmetry may indicate a minor interaction in the past. Overall, the galaxy appears to be a relatively undisturbed, quiescent system.
