This galaxy appears to be a spiral galaxy, likely at an intermediate distance. The disk is slightly inclined with respect to our line of sight, presenting a somewhat elliptical appearance. There is a central bulge that is fairly bright and concentrated. The spiral arms are somewhat flocculent in nature, displaying patchy star formation. There may be a bar-like structure within the central bulge. The galaxy exhibits a bluish hue, which is indicative of ongoing star formation. There may be some faint tidal features present, possibly suggesting past interactions. Overall, the galaxy is moderately bright.
