The galaxy exhibits a predominantly blue hue, indicative of ongoing star formation. Its morphology suggests a disk galaxy, although the structure appears somewhat disturbed, possibly due to a minor or major merger event. Faint spiral arm structures are discernable, emanating from a central bulge region. The bulge itself is of moderate size relative to the overall galactic disk. A weak bar structure may be present across the central region. The disk is observed at a face-on orientation, with little to no edge-on inclination. The overall luminosity of the galaxy, implied by its color, suggests a modest absolute magnitude.
