This galaxy appears to be a spiral galaxy, exhibiting a central bulge and at least one visible spiral arm. The arm appears somewhat disrupted. The light distribution suggests a relatively bright nucleus and a disk that is moderately inclined with respect to our line of sight. The color gradient indicates active star formation regions within the arm, noticeable due to their bluer color compared to the central region. There may be evidence of a minor interaction or tidal disturbance affecting the galaxy's morphology, potentially related to the disrupted arm and the slightly irregular shape of the disk. The redder color suggests it might be a quiescent arm that is not forming as many stars. Overall, the galaxy exhibits characteristics of a spiral system undergoing some form of interaction or internal instability, although no other interacting body is visible in the image. 
