The galaxy presents an overall smooth morphology, though some features are discernible. It is oblong, with a somewhat elongated shape. The galaxy's light distribution appears centrally concentrated, with a noticeable decrease in intensity moving outwards from the core. There is evidence of a possible tidal tail or plume extending from the main body, indicative of gravitational interaction or past merger event. The color is predominantly bluish, suggesting a population of relatively young, hot stars, and ongoing star formation. Some reddening is observed in the core of the galaxy. Based on the morphological features, there are likely some disk-like components in the galaxy. The system appears to be undergoing some form of interaction or disturbance, as evidenced by its irregular shape and potential tidal feature.
