This galaxy exhibits a spiral structure, displaying loosely wound arms that extend from a prominent central bulge. The bulge appears to be moderate in size, contributing significantly to the galaxy's overall luminosity. The disk is clearly visible, oriented at an angle that is not quite edge-on. There is some evidence of disturbance to the galaxy from an ongoing or recent merger with another galaxy, although most voters felt it was a merger. The color distribution suggests active star formation regions within the spiral arms, indicated by a slightly bluer hue. Overall, the galaxy's morphology suggests an intermediate stage of evolution, characterized by ongoing star formation and potential interaction with another galaxy.