The galaxy presents as a spiral galaxy with a moderate inclination relative to our line of sight. Spiral arms are visible, exhibiting a moderate winding, tracing a path around a central bulge. The bulge component appears to be of moderate size relative to the overall galactic disk. Evidence suggests the presence of a bar structure spanning a significant portion of the galaxy’s central region. There may be a minor disturbance in the structure of the spiral arms, possibly indicating a past or ongoing interaction with another galaxy or an internal dynamic event. The light distribution across the galaxy indicates active star formation regions within the spiral arms.
