The galaxy presents as an elongated, cigar-shaped structure, with an apparent bulge at the center. It exhibits a smooth, centrally concentrated light profile, which is a common feature for this morphological type. The outer regions of the galaxy appear fainter, fading smoothly into the background sky, suggesting a gradual decrease in stellar density with increasing distance from the center. The galaxy shows only very subtle disturbances in its form, with a likelihood of interactions, but not showing major disturbances from it. The axial ratio indicates the galaxy is significantly flattened along its minor axis. The color gradients suggests slightly bluer colors toward the outer regions. Overall, the galaxy appears to be a fairly quiescent object, with no indication of strong ongoing star formation within the last 100 million years, which is consistent with the smooth structure and color gradients observed. 
