This galaxy presents a complex morphology, potentially indicative of an ongoing or recent merger event. The primary light distribution appears relatively smooth, suggesting an elliptical-like profile. However, there are clear signs of tidal interactions. Two distinct nuclei or density peaks are visible, implying the presence of at least two interacting galactic components. Faint wisps or extended features are present, hinting at tidal tails or disrupted stellar streams formed during the merger. These features extend outwards from the main body, and their faintness indicates low surface brightness. The color profile appears relatively uniform, with a generally yellowish hue, typical for older stellar populations. There is little evidence of significant dust lanes or prominent star formation regions. The galaxy exhibits a somewhat elongated shape, possibly a consequence of the gravitational interactions.
