The galaxy exhibits a morphology suggesting an ongoing or recent interaction or merger event. The primary component presents a largely smooth, elliptical appearance with a concentrated, bright core. A distinct tidal tail extends outwards from this central region. The tail exhibits a more diffuse, elongated structure, with hints of knots or clumps of material distributed along its length. Color gradients are visible within the galaxy; the core appears more yellow, while the tidal tail tends toward redder hues. This reddening may indicate an aging stellar population or higher dust content in the tail. A significant portion of the light is emitted from a compact, spheroidal central region. The observed shape is highly rounded, with only minor deviations from a perfect ellipse. There is some disturbance in the morphology that is clearly visible. There may be a small merger event taking place.
