The galaxy presents as a disk galaxy, moderately inclined relative to the observer's line of sight. The disk exhibits a degree of internal structure, including a relatively smooth central bulge and some less-well-defined spiral arm segments. The galaxy displays a yellow-orange hue in the central region, suggesting a population of older stars, while the arms have a more reddish hue. The morphological characteristics suggest a potentially ongoing or recent merger or tidal interaction with a smaller companion galaxy, giving rise to a somewhat disturbed or irregular appearance in portions of the disk, and faint tidal tails. Overall, the galaxy's structure indicates a mature system with ongoing star formation activity.
