The observed galaxy exhibits an elongated morphology, approximately 12 arcseconds in its longest dimension. The central region displays a bright, concentrated nucleus, suggesting a high stellar density. The light distribution appears to be dominated by older stellar populations, as indicated by the reddish hue. A fainter, less defined disk-like structure seems to extend from the central region. This structure shows possible indications of disturbance, with some asymmetry and faint features that could indicate interactions. A distinct secondary concentration of light exists to the side of the primary concentration, indicating a close companion. Based on its light profile and disturbed features, the system is likely either undergoing or has recently experienced a merger event.
