The galaxy presents as an elongated, cigar-shaped structure, viewed at a steep angle. Its morphology suggests a possible edge-on spiral or an elliptical galaxy with a significant deviation from a perfect sphere. The central region exhibits a higher surface brightness, appearing smoother and more uniformly illuminated, likely representing the galactic bulge or core. Fainter, diffuse extensions are observed emanating from the central region, potentially indicative of a disk component. There are subtle irregularities present, hinting at possible interactions or minor disturbances. Overall, the galaxy appears relatively smooth, but the structure is not perfectly uniform, suggesting some ongoing or recent dynamic activity.
