The galaxy presents a lenticular, or possibly a spiral structure viewed edge-on. A bright, nearly elliptical bulge dominates the central region, displaying a white-blue color indicative of hotter, younger stars, or possible active galactic nuclei activity. Fainter arms or a disk extend outward, appearing more reddish-orange, suggesting an older stellar population, and a possible significant amount of dust extinction. Some evidence of distortion or tidal features is visible, especially in the edges of the structure, potentially indicative of a minor gravitational interaction or merger event. These features are subtle and would require additional analysis to verify. The galaxy is relatively compact, the overall morphology has some smooth characteristics, but has some visible irregularities.
