The galaxy exhibits a distinct spiral structure, characterized by tightly wound arms emanating from a central region. The arms are not uniformly distributed, with one section appearing more prominent and defined than the others. Within these arms, there appears to be a mottled texture, suggesting regions of active star formation. The galaxy does not appear to be highly inclined relative to our line of sight. The central bulge is subtle. There is also an interaction happening between the spiral galaxy and a less prominent object, which appears to be an area of star formation. The overall color of the galaxy is blue-shifted, indicating a population of relatively young, hot stars. This suggests a relatively recent epoch of star formation. There does not appear to be a strong bar structure. Evidence of interaction with another galaxy or minor disturbance is present.
