The galaxy exhibits a complex morphology suggestive of an ongoing or recent merger event. The primary body of the galaxy appears relatively smooth, with a centrally concentrated bulge exhibiting a yellowish hue, possibly indicating an older stellar population. A fainter, more extended component is visible, displaying a bluer color, implying the presence of younger, hotter stars, perhaps induced by the interaction. The overall shape deviates from a perfect elliptical, presenting some distortion and a suggestion of tidal features. The luminous central region is surrounded by a more diffuse halo. The galaxy appears to have an irregular shape, with a noticeable extension, potentially indicating a disruption due to gravitational interaction with another galaxy.
