The galaxy presents as a spiral type, displaying a disk-like morphology. The galactic bulge appears moderately prominent, exhibiting a yellowish hue indicative of an older stellar population. Two well-defined spiral arms are apparent, loosely wound around the central bulge. The arms are characterized by a bluer color, suggesting the presence of ongoing star formation regions. There is no evidence of major mergers or significant tidal disturbances. The galaxy is observed at an angle, suggesting the presence of a disk and spiral structure. There is also evidence of a bar structure within the spiral arms. The dust lanes appear subtle, distributed along the spiral arms, not significantly obscuring the galactic disk.
