The galaxy presents a moderately bright, somewhat diffuse appearance. It exhibits a complex morphology, suggestive of an ongoing or recent interaction. There appears to be a dominant, rounder component, possibly a bulge, and a fainter, more elongated component. The color profile is broadly consistent with an older stellar population, with a noticeable lack of strong blue light, indicating relatively low ongoing star formation. There is some evidence of tidal features or other distortions. A merger cannot be ruled out.
