This galaxy appears to be a relatively smooth, disk-like structure, although its exact morphology is somewhat difficult to discern due to the image resolution. The galaxy exhibits an elongated shape, leaning more toward an in-between state, showing perhaps a slight cigar shape. The central region is more concentrated and exhibits a yellow-orange hue, suggesting a population of older stars. The outer regions show a gradual decrease in brightness, appearing more diffuse, with slight hints of blue, hinting at areas of recent, or ongoing, star formation. There are no obvious signs of a major merger or significant tidal disturbances. Any interactions are likely minor or not visible at this resolution.
