The galaxy presents as a somewhat faint, disk-shaped structure with a clearly defined central bulge. The disk exhibits a bluish hue, suggesting the presence of younger, hotter stars and ongoing star formation within the spiral arms, if present. It seems to be moderately inclined relative to our line of sight. The galaxy's overall structure is relatively smooth, but there appears to be some minor distortion or asymmetry in the outer disk, possibly indicating a past interaction or minor merger event. The light distribution within the galaxy is uneven, with some knots of brighter emission observed, further suggesting ongoing star formation activity.
