The galaxy presents as a somewhat elongated structure, likely a disk galaxy seen at an oblique angle. A bright, concentrated central bulge is apparent, surrounded by a more diffuse disk. The disk shows some evidence of structure, although distinct spiral arms are not readily visible. There is an irregular distribution of light throughout the galaxy. Patches of bluer light suggest areas of ongoing star formation, while redder regions are suggestive of older stellar populations. The galaxy seems to be experiencing a relatively low rate of star formation. Overall, the galaxy appears to be undergoing some form of disturbance, perhaps a minor interaction or merger, contributing to its irregular shape.
