The galaxy presents an overall elliptical morphology, displaying a relatively smooth light distribution, but some features can be determined. The central region exhibits a concentration of light, indicating a possible bulge. There's a hint of disturbance present in the galaxy's structure, suggesting a minor interaction or merger event in its past. There seems to be a significant star formation rate based on the galaxy's color, though no distinct spiral arms or prominent star-forming regions are evident in this image. The galaxy appears relatively massive.
