The galaxy presents a somewhat amorphous structure, with a suggestion of a central bulge region. The light distribution within the galaxy appears uneven, with some regions exhibiting a more diffuse glow and hints of possible tidal features. The overall color is dominated by yellowish hues. This might imply a stellar population dominated by older stars, though pockets of redder emission are present in the central region. The overall form is suggestive of a merging system or the aftermath of a significant gravitational interaction. The light distribution does not seem to follow a distinct disk or spiral pattern, suggesting a more chaotic morphology.