This galaxy appears to be a spiral galaxy, characterized by a distinct disk structure. The spiral arms are tightly wound around a central bulge. The bulge itself appears relatively small in comparison to the overall disk size. There is evidence of active star formation regions within the spiral arms, indicated by the patchy, somewhat bluer regions. The galaxy is not perfectly symmetrical, with some distortion possibly from interactions. There are no prominent features of ongoing major merger activity. There may be a slight central bar structure visible. Overall, the galaxy presents as a well-formed spiral, likely undergoing star formation and experiencing some gravitational interaction.
