The galaxy presents as a spiral type, exhibiting a prominent disk structure. The spiral arms are well-defined, displaying a relatively open winding pattern. Two dominant spiral arms can be discerned, appearing as broad, sweeping features emanating from the central region. A faint bar-like structure may be present across the core of the galaxy, bisecting the central bulge. The central bulge shows a moderate size in comparison to the disk. Patches of increased luminosity, potentially indicative of star-forming regions, appear along the spiral arms. There may be a presence of some tidal features or disturbances, possibly indicating some degree of past or ongoing interaction with another galaxy. Overall, the galaxy is characterized by its distinct spiral morphology and apparent active star formation within its arms.
