The galaxy appears to be a relatively smooth, centrally concentrated system. There is a bright, unresolved core region which fades to a more diffuse halo structure, likely due to the low image quality. Some asymmetric features can be discerned, suggestive of either internal disk-like components or possible minor disturbances due to an ongoing or recent interaction, but not severe morphological distortions are present. The galaxy is likely a spiral or irregular galaxy, though the image is too indistinct to tell for sure. The galaxy has a moderate mass, indicating a significant but not extreme stellar population. It exhibits a low, but non-zero, star formation rate. The bluer color indicates that star formation is still taking place.
