The galaxy displays a disturbed morphology, potentially indicative of an ongoing or recent interaction. The main body presents a flattened disk structure, viewed at a slight angle, though the high degree of distortion complicates a definitive classification.

Evidence of spiral arm structure is visible, though these arms are not well-defined or symmetric. The light distribution suggests a possible bar feature crossing the central region. There appears to be a significant bulge component, contributing noticeably to the overall luminosity. There are other small, bright knots of light within the galaxy.

In general, the color profile is a mix of bluish-white regions, possibly indicating areas of recent star formation, with yellower areas, possibly older stellar populations. The dust lanes may be present, obscuring parts of the galaxy.
