The galaxy appears as an elongated, disk-like structure with a noticeable central bulge. The color distribution suggests a mix of stellar populations, with a redder hue in the central region, potentially indicating older stars or significant dust obscuration. The outer regions of the disk show hints of bluer colors, which could be due to the presence of younger, hotter stars indicative of ongoing or recent star formation. There appears to be some degree of asymmetry or minor disturbance in the galactic disk, possibly indicating a past or ongoing interaction with another galaxy. There may be loose features around the galaxy or faint tidal tails, which could strengthen the hypothesis of an interaction. The galaxy is tilted at an angle relative to our line of sight, allowing us to observe its disk-like structure. While it exhibits a relatively smooth appearance, there are faint irregular features within the disk.
