The galaxy presents a somewhat elongated morphology, appearing as an oval shape. It exhibits a relatively smooth texture, with subtle variations in color and intensity across its structure. The light distribution appears centrally concentrated, although there is a noticeable disk-like feature present. The colors indicate moderate star formation, but appear muted overall suggesting that it is not particularly active. There appears to be a minor disturbance in the galaxy's structure. There is no clear evidence of a major ongoing merger, but some level of interaction or past merger event is likely responsible for the disturbance. The galaxy appears to be a moderate-mass system.
