The galaxy exhibits a spiral morphology. Two well-defined spiral arms emanate from a central bulge. The arms appear moderately wound, extending outwards from the galactic center. The bulge region displays a yellowish hue, possibly indicating an older stellar population. The spiral arms show a bluer tint, suggestive of ongoing star formation. The galaxy displays an elongated profile, with the disc oriented at a slight angle relative to our line of sight. There may be a slight bar structure in its center. The galaxy appears relatively isolated, with no obvious signs of major interactions or mergers, though some asymmetry in the disk hints at a minor disturbance.
