The galaxy appears to be a relatively small object with a slightly irregular shape. It exhibits a bright central core that fades outwards. The light distribution appears mottled, rather than uniformly smooth. There is some suggestion of a disk or spiral feature. The galaxy displays a blueish hue which could indicate a population of young stars. There appears to be a slight hint of disturbance in its morphology, but no clear signs of a major ongoing merger are visible. The galaxy appears to be an isolated system with no other objects nearby to suggest any interaction.
