The galaxy presents a notably smooth, elongated morphology. Its color profile exhibits a concentration of light towards the central region with a gradual fading toward the outer edges. The central region has a slightly yellowish hue, possibly indicative of an older stellar population. The outer regions appear somewhat bluer, suggesting the presence of more recent star formation, though it's relatively subdued across the galaxy. The overall structure hints at a disk-like formation viewed at an oblique angle. There might be a slight warp or disturbance visible in the outer regions, but further investigation is needed to confirm this. It appears relatively isolated with no obvious signs of major mergers, though there might be a faint tidal tail or stream extending from one end of the galaxy, suggesting a past interaction. Overall, it appears to be a relatively evolved galaxy undergoing a modest amount of star formation.
