The galaxy presents as a dual-component system. One component is elongated, appearing as an edge-on or highly inclined disk galaxy. Its color profile exhibits a gradient, suggesting possible differential reddening or stellar population differences along its major axis. The other component appears more spheroidal in shape, likely an elliptical galaxy or the bulge of a spiral galaxy. It exhibits a smoother, less structured appearance with a yellowish hue, indicative of an older stellar population. There is a possibility of an interaction between these two galaxies based on their proximity to each other, however, further data and analysis are needed to confirm this. No strong tidal features or distortions are immediately apparent. The galaxy is relatively smooth with no obvious merging activity, but it seems disturbed.
