The galaxy presents an elliptical-like morphology, appearing generally smooth with a concentration of light towards the central region. There is some evidence of a disturbed morphology, potentially from a tidal interaction or recent merger event. The primary body shows an elongated shape, with an overall yellowish hue indicative of an older stellar population. A secondary, smaller component is visually distinct and located near the primary component, displaying a bluer color, hinting at ongoing or recent star formation. The system appears to be undergoing a possible merging process.
