This galaxy appears to be a relatively compact object. The core region exhibits a high degree of luminosity, appearing nearly spherical and unresolved in this image. There is a slight extension of the galaxy beyond the core region. The edges of the central bright region are somewhat poorly defined suggesting that the central concentration decreases with radial distance. The outer regions seem to show some irregularity, hinting at possible disturbances. The galaxy presents with a gradient from a bright, almost white core, which transitions to bluer tones in the outer edges. There are subtle hints of redder regions and an overall blue hue at the edges suggesting the presence of younger stellar populations or ongoing star formation in the periphery. Overall the galaxy's morphology points towards a spiral or disk galaxy with a dominant central bulge, potentially undergoing some minor interaction or disturbance event.
