The observed galaxy presents as a disk galaxy, viewed at an angle that is close to face-on. The central bulge appears moderately bright, exhibiting a smooth, concentrated distribution of light. Spiral arm structures are clearly discernible, extending outwards from the bulge, and can be categorized as grand-design. The arms are relatively well-defined, and are composed of distinct concentrations of stellar populations with active star formation regions. These regions exhibit a bluer color than the central bulge, suggesting the presence of younger, hotter stars. Two prominent spiral arms are visible. There is evidence of a bar-like structure within the central region, as the central bright region is clearly elongated. There is a strong likelihood of a merger or interaction with another galaxy sometime in the past, with the galaxy displaying minor structural disturbances.
