The galaxy presents a roughly circular morphology with a bright, concentrated core region. The central area is a dominant feature, exhibiting a high surface brightness. Surrounding the core, there is a fainter, diffuse halo, suggesting a gradual decrease in stellar density with increasing radius. Evidence of some tidal disturbance or recent minor merger. There are no spiral arm structures are readily discernible in this image. The overall colour appears somewhat redder, potentially indicating an older stellar population or significant dust obscuration.
