The galaxy presents as a relatively large spiral galaxy with a notable disk structure. The arms appear well-defined, exhibiting a grand design morphology characterized by two prominent, extended spiral arms. These arms display a moderately open winding pattern, gradually extending outwards from a central region. The galactic bulge is discernible but does not dominate the overall structure, suggesting a moderate size. A bar structure is present, though it appears somewhat weak and not particularly prominent within the central region. There is no strong evidence of any major ongoing merger events, although subtle disturbances could be present in the outer arms. The overall appearance suggests a spiral galaxy with considerable star formation activity.
