The galaxy appears to be a relatively large, elongated spiral galaxy, likely seen edge-on. There is a bright central bulge which dominates the galaxy's overall luminosity. Fainter, diffuse light extends outwards, with a slight blue tint that may be indicative of some star formation within the galaxy's disk. The galaxy shows indications of potential disturbances in its morphology. There is some lopsidedness to the overall structure which could point to a gravitational interaction or recent minor merger event.
