The galaxy appears to be a faint, relatively small object. The light profile suggests it is likely a smooth galaxy with some disturbances. It exhibits a red hue in the optical bands, suggesting a population of older stars or significant dust obscuration. There is slight evidence of possible tidal features that could indicate a minor merger, but further analysis is required to confirm this. Overall, the galaxy presents a morphology that suggests a quiescent and fairly evolved system, though not entirely undisturbed.
