This galaxy appears to be a spiral galaxy with a moderately sized bulge. There is evidence of two distinct spiral arms, indicating a grand design structure. These arms appear to have a medium winding. The galaxy is involved in a potential merger event, appearing disturbed, or potentially showing a more recent interaction with another galaxy, given the uneven and clumpy distribution of light in the disk and possible tidal features. The color gradient suggests a mix of stellar populations, with a generally redder bulge and more bluish arms indicative of ongoing or recent star formation activity. There are subtle irregularities, but it is difficult to determine the magnitude of the disturbance from this image alone. The galaxy has a generally face-on orientation. 
