The galaxy appears as a roughly elliptical, relatively smooth object with a concentration of light towards its center, suggesting a central bulge. A subtle color gradient is observed, with the core exhibiting a yellowish hue, potentially indicating an older stellar population. The outer regions display a bluer tint, which could imply more recent star formation activity, though it is not very pronounced. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape. No distinct spiral arm structures or strong dust lanes are apparent in this image. Based on its general morphology, the galaxy is possibly an early-type spiral galaxy or an elliptical galaxy. It doesn't appear to be undergoing any major merging activity. Overall, the galaxy has a reasonably regular and well-defined structure.
