The galaxy presents as a relatively compact, edge-on disk galaxy. It displays a smooth, elliptical light distribution, indicative of a bulge component. A dusty disk is implied, as the color appears more red. No spiral arm features are readily apparent. The overall color suggests an intermediate age stellar population, potentially with ongoing, albeit possibly low, levels of star formation. The galaxy's high degree of flattening indicates a well-defined disk. The galaxy does not show signs of any major disturbances or ongoing mergers.
