The galaxy presents a disk-like morphology, potentially observed at an angle significantly inclined relative to our line of sight, but likely not fully edge-on. The central region exhibits a concentrated luminosity profile, suggesting the presence of a bulge component. There appears to be some patchiness visible, indicating areas of star formation. The galaxy is relatively large and is undergoing moderate star formation. It displays some signs of disturbance, which may indicate a possible minor merger or interaction.
