The galaxy presents a moderately disturbed morphology, indicative of an ongoing or recent interaction. The primary body of the galaxy exhibits a somewhat smooth appearance, with a central bulge that appears diffuse rather than sharply defined. Faint features extend outwards, appearing as subtle tidal tails and bridges, possibly suggesting a merger event with another galaxy. There is some irregularity and patchiness observed in the light distribution, hinting at localized star formation regions within the galaxy. Overall, the galaxy does not appear to have a well-defined spiral or elliptical structure and is more of an intermediate class with irregular features.
