The galaxy presents a well-defined spiral structure. Two dominant spiral arms emanate from a bright central bulge. The arms appear tightly wound, exhibiting a flocculent morphology with some discontinuity. The galaxy's overall color suggests a mix of stellar populations. The spiral arms show hints of blue, indicating ongoing star formation, while the bulge appears more yellow, suggesting an older stellar population. The disk of the galaxy has a noticeable tilt with respect to our line of sight, though it does not appear to be edge-on. There might be a weak bar feature present across the central region, though it is not prominently defined. The galaxy displays moderate rotational symmetry, without significant signs of major disturbances or ongoing merging activity. The structure is compact with some distortion in the outer edges, indicating possible interactions with another galaxy in its environment.
