The galaxy appears as two distinct, somewhat diffuse, luminous regions. The overall color profile suggests a redder hue, especially towards the core of the galaxy, which may indicate an older stellar population. There is some evidence of a bluer component within each of the two luminous regions, potentially indicative of regions of on going star formation. The general shape suggests a relaxed morphology with little to no signs of strong tidal features, although the two distinct luminous regions may indicate the later stages of a minor merger. There is a lack of strong spiral arm structure or a well-defined disk.
