The galaxy exhibits a prominent disk structure with noticeable spiral arms. These arms display a generally medium winding pattern, suggesting a moderate rate of rotation. A significant fraction of the disk appears to be composed of spiral arms, as opposed to a smooth, featureless structure. There is a central bulge of moderate size, though its overall contribution to the galaxy's light appears less dominant compared to the disk. Evidence suggests the presence of a bar structure, albeit not a particularly strong one. The galaxy exhibits blue color indicative of on going star formation.  There are no obvious signs of a major merger or significant tidal disturbance, though some indications exist of a minor disturbance or interaction. The spiral arm counts is 2.