The observed galaxy presents a primarily smooth morphology, with a centrally concentrated light distribution. It displays an elliptical shape, appearing elongated, but not extremely so. The galaxy exhibits a noticeable color gradient, with a brighter, bluer core region, gradually fading into a dimmer, more diffuse outer halo. There's a subtle suggestion of minor disturbances or irregularities in its form, possibly indicating past or ongoing interactions. The object appears relatively isolated, showing no clear signs of an ongoing major merger.
