The galaxy presents as a relatively faint, elongated structure with a slight blue tint. Its apparent shape is somewhat irregular, possibly indicating a disk galaxy viewed at an oblique angle. There's a suggestion of some smoother, centrally concentrated light, perhaps a bulge. The galaxy exhibits a faint, diffuse halo. There is no spiral structure that can be determined. There may be a tidal disturbance or it could be viewed at an angle. It does not appear to be undergoing a major merger. The overall low surface brightness suggests a relatively low star formation rate, but given its estimated stellar mass, the specific star formation rate appears relatively low.
